The galaxy presents a smooth, elliptical morphology. Its light profile is dominated by a central bulge with a bright, concentrated core. The galaxy exhibits a slight elongation, appearing somewhat cigar-shaped rather than perfectly spherical. There is little to no evidence of spiral arms or prominent disk structures. The color distribution is relatively uniform, with a subtle shift towards redder hues in the central region, suggesting an older stellar population and a lower rate of star formation. No signs of ongoing mergers or tidal disturbances are visible. The outer regions of the galaxy gradually fade into the background.
