The galaxy presents a generally smooth, elliptical morphology. It displays a concentrated central bulge that appears to be the brightest region. Surrounding this central concentration is a more diffuse halo of light, gradually fading into the background. There is some evidence of slight elongation, with the galaxy appearing somewhat cigar-shaped rather than perfectly spherical. The color profile seems to indicate an older stellar population, dominated by redder hues in the central region. The outer halo exhibits a slightly bluer tint, possibly indicating some younger stars, or potentially artifacts of imaging. There is no obvious evidence of ongoing major merger activity or strong tidal disturbances, though it does appear there are some minor disturbances possibly ongoing. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
