The galaxy appears to be an elliptical type. It presents a smooth, generally featureless morphology with a significant fraction of the light concentrated in a central bulge region. The object exhibits an elongated shape, appearing somewhat cigar-shaped, rather than perfectly spherical. The color profile suggests a dominant population of older stars, with a redder hue observed than what is seen in typical spiral galaxies. There's a slight indication of some minor asymmetry or possible tidal disturbances, hinting at a past interaction or merging event, although no major mergers or strong disturbances are apparent. The galaxy has intermediate size.
