The galaxy presents as a somewhat compact object, with an approximate apparent diameter of 9 arcseconds. A central concentration of light is noticeable, possibly indicating a central bulge or active galactic nucleus. There is some structural irregularity, suggesting a moderate degree of disturbance. Weak tidal features are present in the form of a blueish trail on one side of the galaxy and a light colored tail on the other side. These could be indicative of past or ongoing gravitational interactions with other galaxies. The general color appears to be predominantly reddish, with a slight blueish tint in the outer regions. This could suggest an older stellar population with some ongoing star formation. Overall, the galaxy appears to be in a state of flux, likely driven by a combination of internal processes and external interactions.
