The galaxy presents as a roughly elliptical object with a smooth, featureless appearance. Its central region is bright and concentrated, suggesting a high stellar density or the presence of an active galactic nucleus. Moving outwards from the core, the luminosity gradually decreases, with no distinct spiral arms or bar structures visible. The overall color appears relatively red, indicative of an older stellar population and a lower rate of recent star formation. The galaxy's shape is closer to being in between round and cigar shaped. There is no obvious indication of significant tidal disturbances or ongoing mergers with other galaxies, although subtle asymmetries may suggest minor past interactions. 
