The galaxy presents as a centrally concentrated object with an approximately elliptical morphology. The light distribution appears relatively smooth, suggesting a lack of significant spiral arm structure. The central region exhibits a yellowish hue, potentially indicating an older stellar population. The overall color suggests a system dominated by evolved stars and a relatively low rate of current star formation. There are no prominent tidal features or morphological disturbances visible, implying that the galaxy is not undergoing a major merger or strong gravitational interaction.
