The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a centrally concentrated brightness profile, indicating a high density of stars in the core. The light distribution suggests a spheroidal shape, deviating only slightly from perfect roundness. There's no readily apparent disk structure or spiral arms. The color profile is consistent with an older stellar population, displaying a redder hue in the central regions. There is some evidence of faint, diffuse light extending outwards from the main body of the galaxy, suggesting a possible extended halo or tidal features, but these are not pronounced. There do not seem to be any other prominent or major disturbances.
