The galaxy appears as a smooth, elongated object with a concentrated central bulge. The color profile suggests a relatively evolved stellar population, exhibiting a yellowish-red hue. There is no readily apparent spiral structure or significant dust lane obscuration. The galaxy appears largely undisturbed, with no obvious signs of ongoing merger activity or tidal distortions. Its overall morphology is consistent with that of an elliptical or lenticular galaxy seen at an oblique angle. The size is relatively small. The galaxy is centrally concentrated and not very bright.
