The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing elongated with an approximate axis ratio of 2:1. The color profile suggests an older stellar population, with a dominant yellowish hue. There is a smooth radial decrease in light intensity. There is no resolved spiral arm structure visible, nor are there any prominent dust lanes or irregular features indicative of recent major mergers. However, there may be some minor disturbances present. Overall, the galaxy appears to be a quiescent system, with low star formation.
