The galaxy presents a generally smooth morphology, with a dominant central bulge. The light profile is centrally concentrated, exhibiting a gradual decline in surface brightness outwards. Its overall shape appears largely round, with a mild deviation towards a slightly elongated form. Faint, diffuse features suggestive of a possible disk component may be present, though not prominently defined. Subtle disturbances are present, potentially indicating interactions with a smaller galaxy. The galaxy displays colors indicative of a relatively mature stellar population with ongoing star formation. The central bulge emits in the g, r and z bands.
