The galaxy presents as a slightly elongated elliptical shape. A bright, concentrated central bulge dominates the structure, characterized by a yellowish hue suggesting an older stellar population. The surrounding disk appears relatively smooth with a faint, diffuse blue color, which may indicate areas of recent or ongoing star formation, however the galaxy is dominated by redder light suggesting a suppressed star formation rate overall. There are only slight indications of spiral arm structures. The galaxy appears relatively isolated and does not show any obvious signs of major tidal disturbances or ongoing mergers, though some minor asymmetry hints at possible past interaction or internal processes at play.
