The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its core region appears bright and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. The galaxy lacks any visually discernible spiral arm structure or prominent dust lanes. It's overall shape is not perfectly circular but instead a somewhat elongated elliptical shape. The gradient of color, while subtle, indicates a possible redder periphery compared to the central core. There are no obvious signs of tidal disturbances or ongoing mergers. The galaxy appears to be a fairly isolated object in the observed field.
