The galaxy presents as a primarily smooth, elliptical morphology. Its light profile is centrally concentrated, exhibiting a bright, yellowish core that gradually fades into a more diffuse outer region. There is a slight elongation evident in the overall shape, suggesting a transition between a perfectly spherical and a more cigar-shaped structure. The overall color is consistent with an older stellar population, with limited evidence of ongoing star formation regions visible in this imaging. There are no discernible spiral arms or strong tidal features indicative of major interactions. Subtle asymmetry may imply a minor disturbance.
