The galaxy presents as a moderately bright, extended object with an overall elliptical morphology. There appear to be two distinct components, with a clear separation between them.

The upper component exhibits a smoother, more diffuse appearance, with a pale, relatively uniform color. The lower component shows signs of potential disturbances in its structure. This component appears slightly more compact and exhibits a distinctly redder hue than the upper component. This color difference may indicate different stellar populations.

The presence of two components and the apparent disturbances suggests the possibility of an ongoing or recent interaction between the two structures. This interaction could potentially be a minor merger, or tidal disturbances between interacting galaxies. The tidal disturbances could be in the form of tidal tails, plumes, or asymmetries in the outer regions.
