The galaxy presents as a slightly inclined disk galaxy. A prominent central bulge is evident with a relatively smooth texture. The disk structure shows evidence of spiral arm features, although these are not sharply defined. There appears to be a slight asymmetry to the disk, suggestive of possible interactions or internal disturbances. The color distribution indicates a central region dominated by older stellar populations, while the disk shows bluer hues, hinting at ongoing star formation, though at a relatively low rate. There does not appear to be any major ongoing merger event or strong tidal features.
