The galaxy appears as a relatively compact, elliptical structure with a smooth, even light distribution. The core exhibits a slightly brighter, more concentrated region, indicating a possible central bulge. There is little to no evidence of spiral arms or significant disk features. Color gradients are subtle, with the core appearing slightly yellower compared to the outer regions, which are more evenly colored. The overall morphology suggests a galaxy dominated by an older stellar population and a lack of ongoing star formation. No signs of tidal disturbances or interactions with other galaxies are visible. The galaxy presents a classic elliptical appearance, suggesting it is a relatively evolved system.
