The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, elongated with a cigar shape, suggesting a potential classification as an elliptical galaxy. The central region displays a bright, yellowish core, possibly indicative of an older stellar population. The outskirts are less defined, gradually fading into the background sky. There is no obvious dust lane or spiral arm structure visible. Overall, the galaxy displays a lack of significant features or irregularities suggesting that the galaxy is relatively undisturbed. There is no evidence of any recent merger.