The galaxy presents as a relatively smooth, disk-like structure, with an apparent elliptical shape, although moderate inclination prevents precise determination of its true form. The radial color distribution suggests a more concentrated population of older stars towards the central bulge, indicated by the redder hue, with hints of bluer, potentially younger stellar populations in the outer disk region. There is evidence of a possible minor tidal interaction or disturbance, with the suggestion of faint extended features or asymmetries. Given the observed color profile, this galaxy exhibits an intermediate mass range and a relatively low rate of star formation. The structure is not perfectly smooth, implying that this is not a lenticular galaxy.
