The galaxy presents as an elliptical morphology with a smooth, relatively featureless structure. There is a concentrated central bulge that appears yellowish, suggesting a population of older stars. The galaxy's overall shape is elongated, tending towards a cigar-like form. No distinct spiral arms or significant dust lanes are discernible. There is no obvious indication of major merger activity, although a subtle irregularity on one side might suggest a minor disturbance. The galaxy exhibits a redder color index, which is consistent with an evolved stellar population and relatively low star formation rate.
