The observed galaxy presents as a centrally condensed object, exhibiting a bright, concentrated core that diminishes in intensity toward the outer regions. The overall shape is broadly elliptical, showing slight irregularities or disturbances along the outer edge. This may be indicative of tidal interactions with a nearby galaxy. The central region of the galaxy appears predominantly smooth. The outer regions are slightly distorted and appear more diffuse. There is some evidence of a potential minor merger or tidal interaction. Overall, the galaxy appears fairly compact and spheroidal.
