The galaxy presents an elliptical morphology with a high degree of smoothness, indicating a likely early-type classification. Its color profile shows a central concentration of yellow light, suggesting a population of older, evolved stars. There is a subtle gradient of color towards the outer regions, showing a slight reddening, possibly due to increased metallicity or dust content.

There is a small disc-like object that may be an interacting galaxy. There does not appear to be any strong indication of ongoing star formation in the primary galaxy, which is consistent with a low star formation rate. The galaxy exhibits a moderate degree of roundness. There's no clear indication of a major merger or strong tidal disturbances in its immediate environment based on its shape and structure.
