The galaxy presents as an elliptical morphology, exhibiting a centrally concentrated, smooth light profile. A bright, relatively spherical core dominates the overall structure. The galaxy fades gradually outward from this core, with a slight elongation, deviating minimally from a perfectly circular shape. There is a lack of any distinct spiral arm structures or prominent dust lanes typically associated with spiral galaxies. No significant tidal features or obvious signs of ongoing major mergers are readily apparent, although subtle irregularities in the outer regions suggest possible minor disturbances. The galaxy's color appears generally redder, indicative of an older stellar population and a relatively low rate of active star formation.
