The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse morphology without prominent spiral arms or a distinct bar structure. The light distribution suggests a relatively old stellar population, with the central region appearing more concentrated and slightly redder in color, indicative of a higher density of evolved stars. The galaxy's overall shape is elongated, exhibiting a cigar shape appearance. There are no obvious signs of active star formation regions or significant dust lanes, and there are no signs of mergers or tidal disturbances from companion galaxies. The galaxy appears relatively isolated and undisturbed.
