The galaxy presents as a generally smooth and rounded object. There is a centrally concentrated, brighter core region that exhibits a yellowish hue, possibly indicative of an older stellar population. Surrounding this core is a more diffuse halo, displaying a slightly bluer coloration, implying the presence of some younger, hotter stars. There is no visible evidence of spiral arms, bars, or significant dust lanes. The overall morphology suggests an elliptical or lenticular galaxy type. There are no indications of a major ongoing merger event, though subtle irregularities in the outer regions may suggest a possible minor interaction or disturbance in the past. The galaxy appears relatively isolated within its field.
