The galaxy presents as a single, relatively smooth and concentrated object. It exhibits a mostly elliptical morphology, appearing quite round. The light profile gradually decreases from the central core outward, displaying no distinct spiral arm structures or prominent features. There appears to be minimal if any dust obscuration present. The galaxy's color is notably yellowish-orange, suggesting a stellar population dominated by older, evolved stars and a relatively low rate of ongoing star formation. There appears to be no evidence of any major tidal disturbances or ongoing mergers, as the galaxy appears isolated and undisturbed.
