The galaxy presents as a roughly elliptical-shaped structure, exhibiting a relatively smooth overall appearance, though some irregular features are present. There is evidence of a disk-like structure, but it isn't very well defined. The central region appears brighter and more concentrated than the outer regions. The color profile suggests the presence of both older stellar populations in the central region and some younger, bluer stars scattered throughout the galaxy. There is potential for an ongoing or recent minor merger or tidal disturbance due to some structural asymmetry. The galaxy’s low star formation rate indicates a passive or quiescent state. The estimated mass suggests it’s a relatively small galaxy.
