The galaxy presents as a diffuse, elliptical form with an approximate size of 4 kpc. The central region exhibits a notably bright and concentrated luminosity, suggesting a prominent galactic nucleus. The overall color profile indicates a mix of stellar populations, with the core appearing more yellow/white, indicative of older stars, and some distal regions showing hints of redder hues, possibly denoting regions of dust obscuration or ongoing, albeit low-level, star formation. There is some subtle indication of possible tidal disturbances or minor asymmetries in the outer regions, suggesting past or ongoing interaction or merging events. 
