The galaxy presents as a single, somewhat diffuse object with a centrally concentrated brightness profile. It is generally ellipsoidal in shape, though a slight asymmetry is observed along its major axis. The color gradient suggests a concentration of older stellar populations towards the center, with bluer components visible along the outer regions of the galaxy. There is evidence of a possible tidal tail or minor disturbance extending from the main galactic body, perhaps indicative of a past or ongoing interaction. This galaxy appears to be a mid-sized system with evidence of at least some ongoing, albeit potentially low-level, star formation. It displays characteristics that lean toward a relatively smooth morphology, with no obvious strong spiral arm structures or a prominent central bulge. There may be indications of a past merger event, but the system appears fairly relaxed and is not dominated by strong morphological disturbances.
