The galaxy appears as a central, concentrated bulge surrounded by a fainter, elongated disk. The bulge exhibits a yellowish-white color, indicating a likely population of older stars. The disk is bluer in hue, suggestive of ongoing star formation. The galaxy is not perfectly circular, possessing a somewhat elliptical shape. There is no clear evidence of spiral arms or a bar structure within the disk. The galaxy appears relatively undisturbed, without major distortions indicating a recent merger or significant tidal interactions. There may be some minor asymmetry in the outer regions of the disk but, overall, the galaxy has a regular morphology.
