The galaxy presents as a largely smooth, centrally concentrated object with a yellowish-gold hue. The light distribution is highly centrally concentrated, suggesting an elliptical morphology. The galaxy appears nearly circular in projection. There is little evidence of spiral arm structure or significant dust lanes. No obvious signs of ongoing major merger activity are apparent, but a very slight asymmetry could indicate a minor interaction or internal disturbance. The redder color suggests a population dominated by older stars and a relatively low current star formation rate. Based on the apparent color and morphology, this object is likely a massive, evolved galaxy.
