The galaxy presents as a centrally concentrated object with a relatively smooth appearance. It exhibits a roughly elliptical morphology, appearing moderately rounded. The central region displays a bright, yellowish hue, suggesting an older stellar population. Fainter, bluer regions are observed extending from the central bulge, possibly indicating areas of more recent or ongoing star formation. There is some indication of minor tidal disturbances or asymmetries in the outer regions of the galaxy, implying possible interaction with a smaller galaxy or other gravitational influences.
