The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellowish-white hue, suggesting a population of older stars. A slight elongation is observed, deviating from a perfectly circular shape. There is a hint of a possible tidal interaction or minor disturbance on the edge of the disk, though this is not definitively confirmed. Overall, the galaxy appears quiescent with little evidence of ongoing star formation.
