The galaxy appears to be an elliptical galaxy, with a smooth, centrally concentrated light distribution. It is elongated in shape, with a cigar-like morphology. There are no obvious spiral arms or prominent dust lanes visible. The central region is brighter and more concentrated, indicating a possible bulge. The overall color is slightly redder, consistent with an older stellar population and relatively low star formation activity. There might be some minor disturbances hinting at a possible interaction or past merger event, but the overall structure seems undisturbed.
