The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated. The light distribution appears to be elongated, with a roundness that is somewhere in between round and cigar shaped. The central region displays a yellowish hue, potentially indicative of an older stellar population. Fainter, bluer light is seen towards the outer regions of the galaxy, possibly suggestive of a small amount of ongoing star formation. There is no discernible evidence of major disturbances or mergers.
