The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a higher density of stars towards the core, gradually diminishing towards the outer regions. The galaxy is mostly a smooth, concentrated form with very few visible distinct features in its spiral arms. The light from the galaxy appears to be somewhat redder when compared to typical younger spiral galaxies, which could be due to an older stellar population. The overall shape is approaching round, but not quite. There are no obvious signs of major recent mergers or strong tidal disturbances that would significantly disrupt its morphology, though subtle irregularities in the outskirts could be hints of minor interactions.
