The galaxy presents as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. There is a distinct central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. Fainter, bluer light extends outwards from the core region, which may suggest some level of ongoing or recent star formation at the outer edges of the galaxy. The overall structure appears largely undisturbed, without any obvious signs of major mergers or tidal interactions. However, there is a subtle asymmetry that suggests the possibility of minor disturbances or past minor mergers. The object's size, and the lack of distinct spiral arms or a bar structure, point to a lenticular or early-type spiral classification.
