The galaxy presents as a relatively smooth, centrally concentrated object, exhibiting a round morphology. The light distribution suggests a high degree of radial symmetry. The galaxy appears yellowish-white, possibly indicative of an older stellar population and reduced ongoing star formation. There is no discernable spiral structure or prominent dust lanes. Faint extensions or tidal features are not obviously present, suggesting it is not currently undergoing a major merger event. There may be some minor disturbances, which could suggest a past or ongoing minor merger event. The galaxy exhibits a moderate size. 
