The galaxy presents as a smooth, centrally concentrated object with a moderate ellipticity. The overall color gradient shifts from a redder core to bluer outer regions. There are no obvious spiral arms, bars, or prominent dust lanes visible. There is a very slight asymmetry, suggestive of minor disturbances. The galaxy exhibits a centrally dominant bulge component, with a relatively faint extended halo. The morphological classification likely corresponds to an early-type spiral or lenticular galaxy. There appears to be a central redder region surrounded by a less concentrated greenish halo, potentially indicating ongoing star formation.
