The galaxy appears to be a relatively smooth and centrally concentrated object. It exhibits a generally elliptical morphology, tending towards a cigar shape, with a slight elongation visible in one axis. The color profile suggests an older stellar population dominating the light output, with a redder hue centrally and some slightly bluer regions present in the outer areas. There appears to be a minor disturbance or possible interaction occurring, as evidenced by faint asymmetric light distribution surrounding the main body and the proximity of at least two smaller objects.
