The galaxy presents as a spheroid with a smooth, diffused appearance, suggesting an elliptical morphology or a lenticular galaxy seen at a moderate inclination. It has a central, concentrated region of high luminosity that fades gradually towards the outer edges. The color profile indicates a primarily older stellar population with minimal presence of dust lanes. The object appears relatively isolated with a secondary object in the lower right of the image; these may indicate a recent or ongoing interaction that is causing disturbances to the galaxy's structure or triggering star formation. The galaxy does not exhibit obvious spiral arms. Overall, the galaxy appears to be in a relatively evolved state, with minimal ongoing star formation.
