The galaxy presents as a somewhat elongated structure, appearing as an elliptical or lenticular type. The central bulge exhibits a yellowish hue, indicating an older stellar population likely dominated by red giant stars. Moving outward from the center, the color transitions to a bluer shade, suggesting the presence of younger, hotter stars and possibly ongoing or recent star formation activity. There is no distinct spiral arm structure visible. The outer regions of the galaxy appear less defined, with a smooth, diffuse appearance. A small fraction of the light may be attributed to tidal disturbance. The overall appearance points to a galaxy that has likely undergone significant evolutionary processes, potentially including past mergers or interactions with other galaxies.
