The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology with a high degree of central concentration. It exhibits an overall flattened, somewhat cigar-shaped form, but is mostly rounded. The central region presents a bright, concentrated core, suggestive of a possible active galactic nucleus or a dense stellar population. The galaxy exhibits a color gradient, transitioning from a yellow-white hue in the center to bluer tones in the outer regions. There are no clearly defined spiral arms or significant dust lanes visible. No merging or interacting galaxies are observed, although there are slight, subtle disturbances in the outer regions. The star formation rate is low, indicating a predominantly older stellar population.
