The galaxy presents a predominantly smooth morphology, with a concentrated central bulge exhibiting a yellowish hue, indicative of an older stellar population.  A faint disk is suggested, extending laterally from the core, displaying a bluer color profile, which may be due to more recent star formation. The disk appears somewhat asymmetric, possibly indicating minor tidal interactions or internal disturbances. The galaxy is relatively compact in apparent size. There is no obvious evidence of strong spiral arm structures.
