The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, diffuse light distribution with a concentrated central bulge. There is a noticeable color gradient, with the central region appearing more yellow-red, suggesting an older stellar population or higher dust extinction. The outer regions appear slightly bluer, possibly indicating the presence of younger stars, though they do not comprise well-defined spiral arms or star-forming regions. The galaxy appears mostly undisturbed, showing no significant tidal features or indications of a recent major merger event. It is moderately luminous, with a substantial stellar mass, and exhibits a relatively low star formation rate. The overall shape is more elongated than spherical, nearing an in-between stage of elliptical and cigar shaped.
