The galaxy appears to be a relatively smooth, elliptical type, exhibiting a somewhat cigar-shaped morphology. The central bulge is pronounced, displaying a bright, concentrated yellowish-orange hue, suggesting an older stellar population. Extending outwards from the core, the galaxy gradually fades into a less defined halo, characterized by a bluer tinge compared to the central bulge. The overall structure lacks prominent spiral arms or distinct features, although there is a subtle asymmetry in the outer regions, potentially indicating a minor gravitational disturbance or interaction. Based on the elongation, this galaxy is viewed at an angle, not face-on.
