The galaxy presents a largely smooth morphology, appearing as a single, consolidated object. A slight degree of asymmetry is perceptible, with a marginal extension on one side, possibly indicative of a minor interaction or internal structure. It exhibits a generally elliptical shape. There is a faint disk that can be seen with little to no features. The galaxy's color profile suggests an older stellar population; the redder hue indicates a diminished rate of active star formation. No obvious signs of an ongoing major merger are visible, as there are not any significant tidal tails or disrupted structures.
