The galaxy appears to be a relatively smooth, elliptical galaxy with a central bulge that exhibits a higher surface brightness compared to the outer regions. The overall shape approximates a slightly elongated spheroid. There are no apparent spiral arms or prominent dust lanes visible. The color gradient suggests a population of older stars, as indicated by the reddish hue particularly in the outer regions, with a bluer color in the central region that could be indicative of a low level of recent star formation. There are subtle irregularities in the outer isophotes, hinting at possible minor disturbances or interactions with other galaxies.
