The galaxy presents a predominantly smooth morphology, suggesting characteristics of an elliptical or lenticular type. A slight elongation is observed in its shape; it is cigar shaped. There is a central bulge with a yellowish hue, indicating a likely population of older stars. Fainter, bluer regions are present, suggesting some degree of ongoing star formation, however, this activity is generally quite limited. The galaxy is relatively undisturbed, with no signs of a major merger event.
