The galaxy presents as an elongated, disk-shaped structure. A prominent central bulge is apparent, exhibiting a concentrated, yellowish hue, suggesting an older stellar population. The disk component appears relatively smooth, with hints of spiral arm structure, potentially diffuse, and subtle variations in color are visible. The overall color index indicates a mature galaxy with ongoing, albeit possibly low-level, star formation activity. The morphological classification appears to favor an elliptical, although the presence of a slight disk cannot be ruled out. There are very subtle hints of a tidal interaction on the lower end of the galaxy. The general form of the galaxy appears relatively undisturbed suggesting no ongoing major merger events.
