The galaxy presents as a relatively smooth, centrally concentrated system. The light profile appears spheroidal, with a noticeable core exhibiting a yellowish hue, suggesting an older stellar population. There is very little to no evidence of spiral arm structures or significant dust lanes. A faint, diffuse halo surrounds the central region. There are no significant tidal features to indicate a recent major merger event, with the overall morphology implying a lack of ongoing, significant star formation. The galaxy has a relatively compact appearance. The shape appears roughly circular, with no strong indications of elongation or asymmetry. The color of the halo is a subtle blue indicating some on-going star formation.
