This galaxy appears to be a relatively smooth, centrally concentrated system. It presents a generally elliptical morphology, deviating slightly from a perfect circle but not exhibiting a distinctly elongated or cigar-like shape. There is a clear central bulge, which dominates the overall luminosity. The outer regions of the galaxy show a gradual decrease in brightness, indicating a lack of distinct spiral arms or other prominent structural features.

There is evidence of some disturbance or interaction. The galaxy does not appear perfectly relaxed; subtle asymmetries or irregularities are visible in its outer regions, suggesting a potential minor interaction or ongoing merger. The colors suggest a mix of stellar populations. The yellowish-white hue of the bulge implies a population of older, relatively passively evolving stars.
