The galaxy appears as a central, roughly circular, luminous concentration. The light distribution suggests a relatively smooth profile, with a gradual decrease in intensity from the core outwards. The overall color is slightly redder than the surrounding field, implying a population of older stars and/or significant dust content. There is no apparent spiral structure or bar feature visible. The galaxy does not seem to display signs of major interaction or significant tidal disturbances, though there is a hint of faint asymmetry in the outer regions. The central core exhibits a relatively high surface brightness.
