The galaxy presents as a moderately bright, lenticular-like structure with a smoothly distributed light profile. The object appears to be an elliptical type, with a slightly elongated shape.  Color gradients indicate a possible aging stellar population, with a faint reddish core. There is no apparent disk-like structure, no spiral arms, and no prominent dust lanes are observed. The overall appearance suggests a galaxy undergoing moderate star formation within the core, however no active galactic nucleus is identifiable from this data. There are no signs of any ongoing major mergers or tidal disturbances.
