This galaxy presents as a single, concentrated light source with a primarily smooth morphology. The core is relatively bright, exhibiting a yellow-orange hue, likely indicative of an older stellar population. A faint, more diffuse halo extends from the central region. The overall shape appears roughly elliptical, with a minimal disk structure. There are no obvious signs of tidal disturbances or ongoing major mergers with other galaxies. Faint bluer regions may indicate small pockets of more recent star formation, although the overall color profile points to relatively low star formation activity.
