The galaxy presents as a generally smooth object, with a slight degree of asymmetry in its overall shape. The light distribution appears centrally concentrated, with a gradual falloff in surface brightness towards the outer regions. The color profile suggests an older stellar population, indicated by the redder hues. There is no obvious indication of a prominent disk component, spiral arms, or active star formation regions. The galaxy does not appear to be undergoing a major merger, but some signs suggest there might be minor disturbances. It exhibits a moderate degree of roundness, leaning more towards an elliptical morphology than a highly elongated or cigar-shaped one. 
