The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge that appears slightly elongated along a vertical axis. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct dust lanes. A faint, diffuse halo surrounds the central region, extending outwards in all directions, but diminishing in brightness with increasing radius. There is evidence of possible minor disturbance or interaction given the slight irregularity in the outskirts. The color profile suggests a population of older stars, with a yellowish or reddish hue dominating the galaxy's overall appearance. The relatively smooth morphology is characteristic of an evolved stellar population and suggests little recent merger activity.
