The galaxy appears as a relatively smooth, centrally concentrated object. There is no obvious spiral arm structure or prominent dust lanes visible. The light profile suggests a spheroid-dominated morphology, consistent with an elliptical or lenticular galaxy. The galaxy exhibits a radial color gradient, appearing more yellowish-orange towards the center, possibly indicating an older stellar population with a larger proportion of red giant stars. The outer regions are more indistinct and diffuse. There are no signs of tidal tails or significant morphological disturbances, which suggests that the galaxy has not undergone a major recent merger. Based on the overall appearance, this galaxy can be broadly classified as an early-type galaxy.
