The galaxy presents a somewhat asymmetric profile, with a brighter central region. Its overall morphology is relatively smooth, with a subtle disk-like structure visible, though some asymmetry is present. There is no clear spiral arm structure that can be discerned. Faint features suggestive of minor disturbances or tidal effects can be seen around the galaxy, potentially indicative of past or ongoing interactions. The color profile suggests a mixture of stellar populations; the central region shows a blue color, possibly due to ongoing star formation activity, while outer regions appear redder, potentially indicating an older stellar population.
