The galaxy appears as a centrally concentrated object, exhibiting a smooth light distribution. There is no obvious spiral arm structure or distinct features indicative of active star formation regions. The morphology seems largely spheroidal, appearing round with a slight deviation toward intermediate ellipticity.

The core exhibits a yellowish hue that graduates into a redder tint in the outer regions. This color gradient suggests the presence of an older stellar population, particularly within the galaxy's bulge. The smooth appearance of the galaxy suggests that it might be an elliptical galaxy. There is no obvious evidence of ongoing merging activity or major tidal disturbances. There is a lack of pronounced dust lanes or patchiness within the visible light.
