The galaxy presents as a generally smooth object with a somewhat elliptical morphology. There appears to be a slight disk-like structure, though it is not sharply defined. The central region exhibits a bright, concentrated luminosity profile. Subtle irregularities are present, suggesting a minor disturbance, possibly due to a past interaction. Color gradients are subtle but indicate bluer hues in the central region, possibly indicative of ongoing star formation, shifting towards redder tones toward the outer regions. The galaxy is relatively isolated, not displaying any obvious signs of major mergers or intense tidal interactions in the immediate vicinity.
