The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. It is elongated, approximately cigar-shaped, with a dominant central bulge that displays a reddish-orange hue, suggesting an older stellar population with relatively little ongoing star formation. The lack of distinct spiral arms or prominent dust lanes further supports its classification as an elliptical galaxy. The galaxy appears relatively isolated, with no obvious signs of major tidal distortions, mergers, or significant interaction with other galaxies. Some evidence of a possible minor disturbance is present. A slight asymmetry in the extended halo is noted with the possible formation of a tidal tail on the right side of the galaxy. Based on its color and shape, this galaxy is likely a relatively massive, evolved system.
