The galaxy presents a primarily smooth morphology, exhibiting a high degree of central concentration. Its shape is approximately round. The light profile suggests a dominant bulge component, with a gradual decrease in surface brightness outwards. There is a subtle color gradient, with the central region appearing more yellow-reddish compared to the outer parts which possess a faint blue-green hue. This suggests a population of older stars concentrated in the bulge and perhaps some recent, weak star formation in the outer regions. No distinct spiral arms or bar structures are visible. There is no evidence of a major ongoing merger, though there might be a subtle hint of a minor interaction or disturbance in the galaxy's halo.