The galaxy presents as a centrally concentrated, relatively smooth structure. The dominant color is a warm, yellowish-orange in the core region, suggesting a population of older stars. The outer regions exhibit a greenish hue that indicates the presence of ongoing, low level star formation. Overall, it does not appear to have any large scale active star formation. The galaxy lacks any obvious spiral arm structure or prominent features indicative of a recent major merger. The slight asymmetry suggests that the galaxy may be involved in a minor interaction or disturbance.
