The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its light profile indicates a relatively featureless structure, dominated by an elliptical form. The radial distribution of light suggests a bulge-dominated system. The galaxy exhibits a color gradient, with a slightly redder hue in its central regions. The overall color suggests an older stellar population. There is no immediately discernible evidence of spiral arms or significant dust lanes. Minor asymmetries in the light distribution may be present, but are not pronounced, suggesting a possibility of past minor disturbances, but there are no current, ongoing mergers. The round to cigar shape suggests its more closer to in between round and cigar shape. The light fall off is gradual.
