The galaxy presents as a somewhat diffuse, centrally concentrated object. It appears largely featureless, with a smooth light distribution. The core region exhibits a yellowish hue, suggesting a potentially older stellar population. Moving outwards, the color transitions to a more blueish tinge, possibly indicating the presence of younger, hotter stars in the outer regions. There is a hint of a possible disk structure but its features are indistinct. There is no strong evidence of any recent major merger events or significant tidal disturbances. The overall morphology suggests an intermediate stage between a purely elliptical and a spiral galaxy, possibly a lenticular galaxy.
