The galaxy presents as a fairly smooth, elliptical structure with a concentrated central bulge exhibiting a yellowish hue, likely indicative of an older stellar population. There is a subtle, greenish halo surrounding the core, possibly representing a region of ongoing, albeit weak, star formation. The overall morphology appears largely undisturbed, with no obvious signs of recent major mergers or tidal interactions. The galaxy appears quite round, and the color gradient indicates a gradual transition from the luminous core to the fainter outer regions. There might be very faint spiral arms, but this is unlikely.
