The galaxy presents as a relatively small and compact object. Its overall morphology appears somewhat disk-like when considering its axial symmetry, however, the disk is not clearly defined. The galaxy is dominated by a bright, smooth central bulge, which contributes significantly to its overall luminosity. Fainter extended features, likely spiral arms, are suspected but only subtle disturbances or faint hints are present. The central bulge's color suggests younger, bluer stars or high rates of star formation may be dominant here. However, more detailed spectral analysis is required to confirm this, as the colors are not uniform. The outer regions have a redder color, suggesting older stars or higher dust content. There is a suggestion of minor tidal distortion, or possible merging activity occurring with a smaller companion, indicated by faint asymmetry or slight displacement from an elliptical profile. No strong evidence of a major ongoing merger is apparent. Further high-resolution imaging and spectroscopy are needed for a thorough characterization.
