The galaxy presents as a somewhat centrally concentrated, lenticular-like system. It displays a relatively smooth overall morphology, with a bright yellowish-white core indicative of an older stellar population. A fainter, bluish disc-like structure appears to surround the central bulge, suggesting the presence of some ongoing star formation. There is a slight extension of the disc along one axis, but the overall shape is closer to round than elongated. There is no visible evidence of a major merger, tidal tails, or strong disturbances in the galaxy's structure. The galaxy seems to be in a relatively quiescent state. Faint reddish spots within the disc might indicate localized regions of recent star formation.
