The galaxy presents a largely smooth morphology, exhibiting a concentrated central bulge. The overall shape appears close to round. Faint, diffuse features extend outwards from the core, but there is an absence of defined spiral arm structure or a clear disk component. The galaxy displays a colour gradient, transitioning from a bluer hue in its core region to redder colours towards the periphery. This suggests a concentration of younger, hotter stars in the central region with older stellar populations dominating the outer regions. There is no indication of any major mergers or strong tidal disturbances. Faint hints of possible minor disturbances are visible.
