The galaxy appears as an elliptical or lenticular system, exhibiting a smooth, centralized concentration of light. The core region is particularly bright, gradually diminishing in intensity towards the outer edges. There is no apparent spiral structure or prominent dust lanes visible, giving it a generally featureless appearance. The galaxy displays a slight elongation, with the light distribution indicating it may be more cigar-shaped than perfectly round. There are no obvious signs of tidal disturbances or ongoing major mergers. The color profile appears relatively uniform across the galaxy, suggestive of an older stellar population and subdued star formation activity. Overall, the galaxy presents itself as a relatively quiescent system.
