The galaxy presents a predominantly elliptical morphology. The central bulge appears bright and concentrated, exhibiting a smooth, yellowish-white color, indicative of an older stellar population. There is a faint, diffuse halo extending outwards from the central bulge. A slight asymmetry or irregularity is suggested in the outer regions, potentially indicative of a past or ongoing minor merger event or tidal interaction, with a hint of disturbance. There is a notable absence of distinct spiral arms.
