The galaxy appears as a predominantly smooth, elliptical structure. Its core exhibits a high degree of concentration, with a bright, compact nucleus transitioning to a less luminous, diffuse halo. The galaxy presents a largely spheroidal morphology, approaching a round shape, with little evidence of significant disk features or spiral arms. There is no obvious indication of ongoing major merging activity, although some minor disturbances may be present in the outer regions. The color profile suggests an older stellar population, with a greater proportion of redder stars. The galaxy exhibits a moderate size for an elliptical galaxy, and it is at an intermediate distance. The stellar formation rate is relatively low.
