The galaxy presents as a centrally concentrated object with a relatively smooth overall appearance. The central bulge exhibits a bright, yellowish hue, indicating a population of older stars. The galaxy's light profile appears largely elliptical, with a high degree of circularity. There's a hint of a surrounding disk, extending outwards from the core, with a bluer tinge, likely signifying younger stellar populations within these regions.

No significant disturbances or indications of major mergers are immediately apparent in the galaxy's morphology. There may be a subtle asymmetry present in the outer disk, possibly suggestive of a minor gravitational interaction or tidal disturbance. The galaxy's overall structure indicates it's likely an early-type spiral or lenticular galaxy, possibly undergoing a transition.
