The galaxy presents as an elliptical-like structure with a relatively smooth light distribution, suggesting a lack of prominent spiral arms. The core region exhibits a high concentration of light, appearing nearly spherical. The galaxy displays a mixture of stellar populations. The central bulge appears yellow-white indicating older stars, while there is evidence of star formation regions, as indicated by the presence of reddish-orange colors on the edges of the galaxy, suggesting recent or ongoing star formation. There appears to be a faint and diffuse halo surrounding the main body of the galaxy. The overall shape is somewhere between round and elliptical, with the galaxy leaning towards a more rounded appearance. There is a suggestion of tidal disturbances or interaction with another galaxy; this is supported by the presence of disrupted regions along the periphery of the main body. It is possible that there is ongoing or recent merging activity.
