The galaxy appears as an elliptical-type galaxy, exhibiting a smooth, spheroidal morphology. It demonstrates a high degree of circularity, with only a slight deviation towards an elongated shape. The galaxy's color profile indicates a population of older stars, dominated by redder wavelengths in the central region transitioning to slightly bluer tones towards its outer edges, suggesting the possibility of ongoing, albeit subdued, star formation activity in the extended galactic halo. There is no evidence of significant spiral arms, bars, or prominent dust lanes. The galaxy appears relatively undisturbed, with no visible signs of major mergers or interactions with other galaxies, however there is a small disturbance on the left side of the galaxy, suggesting possible interaction.
