The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and featureless morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge component. The galaxy's shape is somewhere between round and elliptical, showing a slightly elongated form. The color profile indicates a relatively evolved stellar population, with a redder overall hue. There is no significant evidence of spiral arms or active star formation regions, indicating a lack of substantial recent or ongoing star formation activity. The galaxy appears relatively isolated, without signs of major interaction or ongoing merger events, though some minor disturbances are possible.
