This galaxy exhibits a morphology suggestive of an early-type system, possibly an elliptical or lenticular galaxy. Its light profile appears relatively smooth and centrally concentrated with little to no apparent spiral arm structure. The overall color index indicates a population of older stars, as it leans towards the redder end of the spectrum. There's also some evidence of recent or ongoing interaction or disturbance. There's some distortion in the galactic profile, which could suggest tidal effects from a companion or a past merger event, and a possible tidal tail is hinted at. The galaxy's inferred size suggests it may be a relatively massive system. Given the observed star formation properties, the galaxy exhibits relatively low but non-negligible star-formation.
