The galaxy presents as a relatively compact object, approximately 6 kiloparsecs in effective radius. Its overall morphology appears smooth and elliptical, exhibiting a noticeable central concentration of light that gradually fades towards the outer regions. There is some indication of tidal features which could indicate an ongoing merger, or recent interaction. The color profile leans towards the redder end of the spectrum, suggesting a population of older stars and a relatively low rate of star formation. Overall, it seems to be a galaxy in transition, perhaps evolving from a more active star-forming state.