The galaxy presents as a roughly elliptical form, with a smooth, diffuse light distribution. The core appears somewhat brighter than the outer regions, with the light gradually fading towards the edges. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. There is subtle evidence of possible dust lanes or other substructure, but they are not prominent. Overall, the galaxy appears to be a relatively undisturbed system. The color suggests a mix of stellar populations, with a possible bias toward older, redder stars. There is little indication of active star formation within the observed area.
