The galaxy presents as a spheroid with a smooth light distribution, characterized by a central bulge that is brighter and more concentrated. This bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy fades into a less defined halo exhibiting a bluish tint.

The morphology appears to be intermediate between a perfectly circular shape and an elongated form, possibly resembling a cigar shape. Indications suggest an interaction event is in progress, as the observed tidal disturbances can be identified. There may be a secondary object in the lower portion of the image that could be either a companion galaxy or part of an ongoing merger.
