The galaxy presents as a centrally concentrated elliptical morphology, with a smooth, diffuse light profile diminishing outwards. The core region is the brightest, exhibiting a near-spherical shape with a yellowish-white hue, suggesting an older stellar population. Fainter, bluer extensions are observed, indicating a possible ongoing, though relatively low, level of star formation within its extended halo. There are some minor disturbances observed in the outer edges, suggesting possible minor gravitational interactions or past mergers. Overall, the galaxy appears to be a relatively isolated system, with a significant spheroidal component.
