The galaxy presents as a concentrated, centrally brightened object with a generally smooth appearance. There is no clear spiral arm structure or bar visible. The galaxy exhibits a somewhat elliptical morphology, although it is not highly elongated. Faint irregularities are suspected in the outer regions. The color profile suggests a predominantly older stellar population. There appears to be minimal evidence of on-going major merger activity; however, some subtle signs may indicate minor gravitational interaction or tidal disturbance. The estimated size suggests a large galactic structure.
