The galaxy appears as a generally smooth, centrally concentrated object. There is a subtle hint of a disk-like structure, although the overall morphology is dominated by its smooth appearance. The galaxy exhibits a slight elongation, not perfectly circular, but also not highly elongated.

There may be some minor disturbance within the galaxy's structure or nearby. This may indicate an interaction with another nearby object or an internal process that might be a possible merger.

Color-wise, the galaxy presents a gradient, shifting from bluer tones in the outer regions toward redder hues in the central core. This color difference could be due to varying stellar populations, with a higher prevalence of younger, bluer stars in the galaxy's outskirts and older, redder stars concentrated towards the center. The presence of a redder core could also indicate significant dust obscuration in the central region, potentially associated with past or ongoing star formation activity.

The galaxy appears relatively isolated in its immediate vicinity, there are no clearly defined companions or tidal features that are present in the image.
