The galaxy presents a moderately bright, somewhat compact appearance. Its morphology appears to be largely spheroidal, with a smooth light distribution. There is no clear evidence of spiral arm structure or a prominent disk. The color index suggests the presence of a relatively evolved stellar population, with a bias towards redder wavelengths. The galaxy exhibits little sign of recent or ongoing major merger activity. Based on the observed features, the object appears to be an elliptical galaxy or an early-type spiral galaxy seen at sufficient distance that its spiral arms cannot be resolved. There is only some slight suggestion of internal structure, indicating either minor disturbances or internal dust lanes.
