The galaxy appears as a moderately luminous, slightly elongated structure. It exhibits a relatively smooth overall morphology, with some suggestion of a central bulge. The colour profile indicates a generally older stellar population throughout the galaxy, with a possible concentration of younger, bluer stars in the outer disk region. There are some suggestions of minor structural disturbances. No well-defined spiral arms are observed. The galaxy presents an intermediate ellipticity and appears to be transitioning between a spheroidal and disk-like morphology.
