The galaxy presents a generally smooth morphology, appearing largely featureless upon visual inspection. It exhibits a centrally concentrated luminosity profile with a gradual decrease in brightness outwards. There's a subtle elongation, though the overall shape is close to circular. The color appears to be a yellowish-white, which may indicate a population of older stars and reduced recent star formation activity. There are no distinct spiral arms or other large-scale structures readily apparent. Subtle hints of bluer light are present in the outer regions. There is no strong evidence of a major ongoing merger or significant tidal disruption.