The galaxy presents as a relatively smooth, elliptical morphology. There is no significant evidence of spiral arms or a well-defined disk structure within this observation. The light distribution appears fairly concentrated, suggestive of an older stellar population. The galaxy exhibits a yellow/orange hue, which is consistent with a population of older, cooler stars dominating the light output.

A possible merging event is observed via the slight irregular shape and faint tidal tail, located to the galaxy's left. This potential interaction with another galaxy could be indicative of a recent or ongoing merger. The overall structure is generally smooth and consistent with an elliptical galaxy in the process of accretion.