The galaxy appears to be an elliptical galaxy, characterized by its smooth, featureless morphology. It exhibits a high degree of roundness, showing no obvious disk-like structures or spiral arms. There is no evidence of any major or minor disturbances in its structure, nor does it seem to be currently undergoing a merging event.

The galaxy's core appears to be quite bright, suggesting a high concentration of stars in that central region. The color profile indicates a slightly bluer hue in the core which transitions to a redder appearance in the outer regions. This color gradient might imply a difference in stellar populations, with younger, bluer stars concentrated in the center, and older, redder stars residing in the outskirts. The size of the galaxy suggests a substantial physical extent.
