The galaxy appears to be an elliptical galaxy, characterized by its generally smooth and featureless morphology. The galaxy displays a central bulge that exhibits a bright, concentrated luminosity, indicative of a high stellar density possibly housing a supermassive black hole. The overall color profile suggests a population dominated by older stars, evidenced by the reddish hue, with a subtle hint of bluer light in the central region, which could indicate recent or ongoing, but subdued, star formation. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy is largely symmetrical, and displays no major disturbances in its structure. The absence of pronounced tidal tails or irregular shapes suggests it is not currently undergoing a major merger event, although there is very faint evidence of minor disturbances. The isophotes exhibit a slight elongation.