The galaxy presents as a centrally concentrated spheroid. The core exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. The overall shape tends towards round, however subtle irregularities exist. There may be a hint of a disk-like structure or faint feature extending outward from the central bulge on one side. The galaxy appears relatively isolated, without evidence of significant tidal interactions or ongoing mergers, although minor disturbances can't be ruled out. Based on the color, size and shape it likely has a substantial stellar mass and modest to little star formation.
