The galaxy presents as a relatively smooth, elliptical morphology. A subtle central bulge is visible, exhibiting a concentration of light in the core region. The galaxy appears elongated, but generally has a rounded shape. There is very little evidence of spiral arm structure or distinct dust lanes. The light distribution suggests a moderate degree of homogeneity, and the absence of strong irregularities indicates it is likely not undergoing a major merger event or showing evidence of significant tidal interactions. The color gradient suggests an older stellar population. There are no visible star-forming regions.