The galaxy appears as a relatively compact, somewhat diffuse object. There's a hint of elongation or perhaps a very faint, disturbed disk structure, though not clearly defined. The central region seems brighter, suggesting a concentration of stars or possibly an active galactic nucleus (AGN), though this is difficult to determine from a single image.

Overall, the light distribution is relatively smooth, though the presence of any fine structures like spiral arms or dust lanes cannot be ascertained. It appears to be relatively isolated, with no immediately obvious signs of major ongoing interactions with other galaxies. The color profile suggests that the galaxy is primarily composed of older stars. There might be a slight redder hue, consistent with an elliptical galaxy or a spiral galaxy with an older stellar population and low star formation rate.
