The galaxy presents as a lenticular or possibly an elliptical galaxy, viewed at a significant angle. Its light profile is smooth, with a concentrated, yellowish central bulge. The overall shape is elongated and cigar shaped. There's a suggestion of a disk component extending beyond the central bulge, exhibiting a bluer hue, most apparent at the far extents, indicating some star formation activity, though seemingly at a low rate. There's no obvious evidence of spiral arm structure or significant dust lanes. No major ongoing mergers or major disturbances are apparent in its morphology.
