The galaxy presents as a somewhat elliptical, relatively smooth structure. The central bulge exhibits a yellowish hue, suggesting a population of older stars. Progressing outwards from the core, the luminosity decreases and the color transitions to a bluer shade. There is no apparent presence of spiral arms or a distinct disk. Faint, diffuse extensions are potentially present. No obvious signs of active galactic nuclei or intense star formation regions are visible. There are no visual indications of a major ongoing merger, although the possibility of minor disturbances cannot be ruled out. The galaxy displays a concentrated central region with gradually fading outer edges, typical of an early-type galaxy.
