The galaxy appears to be a relatively smooth, elliptical system. The central region displays a concentrated luminosity, indicating a prominent nucleus or bulge component. The overall color is slightly redder, suggesting an older stellar population dominating the light output. There is a faint, diffuse halo extending outwards from the core, but no distinct spiral arm structures are visible. There is no apparent evidence of ongoing major mergers or tidal disturbances, though there may be some minor asymmetry in the outer halo. The galaxy presents a nearly circular appearance. Star formation activity appears to be relatively low.
