The galaxy presents as an elliptical morphology, exhibiting a relatively smooth and featureless appearance. The central bulge appears prominent, displaying a concentrated luminosity. The galaxy has a mild disc shape, with a small amount of visible distortion and/or tidal features. There is evidence of a minor interaction event nearby, indicating a potential minor merger in progress. Color gradients suggest a predominantly older stellar population. The galaxy exhibits a noticeable red-shift, indicative of substantial distance.
