The galaxy presents a largely smooth, centrally concentrated morphology. There is little evidence of spiral arm structure or distinct features; the overall impression is of a spheroid. The galaxy exhibits a radial color gradient, with a yellowish core transitioning to redder hues in the outer regions. This could be indicative of an older stellar population in the central bulge with ongoing or recent star formation occurring within the galaxy. There is no obvious indication of any major mergers or significant tidal disturbances in this image, however, this could also be due to resolution constraints.
