The galaxy presents as a relatively compact, though somewhat diffuse, object. It appears to be dominated by a centrally concentrated bulge, exhibiting a smooth light distribution, with a relatively small diameter of about 5 kpc. Color gradients are apparent within the galaxy. The core region displays a yellowish-orange hue, suggesting an older stellar population. A bluer, less concentrated region is seen below the orange core, which may represent a more active star-forming region, though the star formation rate is likely low. There are no clear signs of a spiral arm structure or strong tidal features in the galaxy's immediate vicinity. While there are no obvious signs of any other major disturbances, about 13% of citizen scientists noted a merger. The galaxy presents as a relatively isolated system. 