The galaxy appears to be an elliptical type, presenting a relatively smooth and featureless light profile. It exhibits a slight elongation, deviating from a perfectly circular morphology, but is tending more towards an elliptical form. There is no distinct spiral arm structure apparent. The galaxy's core appears slightly more concentrated than the outer regions. There's no evidence of ongoing major merger activity. The overall color suggests an older stellar population, with a redder hue dominant. The galaxy shows evidence of some disturbance or minor merger.