The galaxy presents as a relatively smooth, centrally concentrated object, displaying a nearly circular morphology. Its light is dominated by a yellowish hue in the central region, indicating a population of older stars. A faint halo surrounds the central area, gradually fading into the background. There is no apparent spiral structure or strong evidence of active star formation. The overall structure suggests a lack of significant recent merger activity. The galaxy seems to be a relatively quiescent system.
