The galaxy presents a generally smooth, elliptical morphology. The core is bright and concentrated, exhibiting a yellowish hue, possibly indicative of an older stellar population. A faint, diffuse halo surrounds the central region, appearing slightly elongated. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall structure suggests a relatively evolved system, potentially a quiescent galaxy with a low star formation rate. The colors suggest a higher concentration of older stars. 
