The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a concentrated, bright luminosity, suggesting a high density of stars. A color gradient is observed, with a yellowish-white core transitioning to a slightly redder hue towards the outer regions. There is minimal evidence of spiral arms or prominent dust lanes. The overall structure appears relatively undisturbed, showing no significant signs of ongoing mergers or tidal interactions. A slight elongation is noted, deviating from a perfectly circular shape, but the aspect ratio suggests it is closer to round than cigar shaped.
