The galaxy presents as a relatively smooth, elliptical-like structure with no apparent spiral arms. Its color profile suggests a population of older stars, with a general yellowish hue indicating a lack of significant ongoing star formation. The galaxy is moderately luminous, with a concentrated core region that decreases in brightness towards the outer edges. There is a slight asymmetry, with the light distribution being more extended in one direction. No distinct dust lanes or other prominent features are discernible, indicative of a relatively quiescent galaxy. There is no evidence of significant tidal interactions or major mergers. The roundish shape of the galaxy suggests it may not be a spiral galaxy.
