The galaxy presents an approximately elliptical morphology, appearing relatively compact with a smooth light distribution. The core region exhibits a high surface brightness, suggesting a concentrated central bulge. The color gradient transitions from a bluer hue in the central regions to a slightly redder color in the outer edges, which could indicate variations in stellar populations or dust content. There is a subtle asymmetry in the outer regions. The galaxy does not appear to display prominent spiral arms or a well-defined disk structure. No clear evidence of a major ongoing merger is readily apparent, however there are possible signs of minor tidal disturbances in the outskirts of the galaxy, indicating some past or ongoing gravitational interactions.