The galaxy presents as a smooth, elliptical-like structure. The light distribution appears relatively even, with a concentrated central bulge. Coloration suggests an aging stellar population, with dominant yellow-red hues. There is a subtle color gradient indicating potentially higher concentration of younger stars in the disk. The overall morphology appears undisturbed, with no obvious signs of recent mergers or tidal interactions. The galaxy displays a notable deviation from a perfectly round shape, appearing more elongated and cigar shaped. This suggests the galaxy may be an elliptical galaxy. The object appears as an isolated system with no other galaxies close by.
