The galaxy presents as a relatively smooth, elliptical structure. The central region exhibits a bright, concentrated core, suggesting a high stellar density. Moving outward from the core, the light intensity gradually decreases, with the isophotes appearing mostly regular.

The overall color is dominated by a yellowish-white hue, indicative of an older stellar population. There is a subtle hint of bluer tones on the outer edges, possibly suggesting some ongoing star formation. However, this blue component is faint and not very extended. The shape appears somewhat elongated, but not extremely so, closer to an elliptical shape.

There is no strong evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed. No obvious signs of a major merger event or tidal interactions with other galaxies are discernible from the image. The morphology generally suggests a relatively evolved system.
