The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with minimal discernible substructure. Its color profile suggests an aging stellar population, dominated by redder hues. There is no clear evidence of a prominent disk or spiral arms. The overall shape is generally elongated, but not significantly cigar-shaped; it falls somewhere between round and elongated.

There are no apparent signs of ongoing major mergers or strong tidal disturbances. The galaxy appears relatively undisturbed, with a structure indicative of a relaxed system. There might be some minor disturbances, however, due to a possible interaction with the nearby galaxy, or some internal instability.
