The galaxy presents as an elliptical-like system, exhibiting a smooth, centrally concentrated light distribution. The core region appears bright and yellowish, suggesting a population of older stars. Moving outward from the center, the color transitions slightly to a bluer hue within the galaxy's halo. This may indicate the presence of a younger stellar population, though the overall color profile suggests a galaxy dominated by older stars. There is little to no evidence of spiral arm structures or dust lanes; the system appears relatively undisturbed. Faint extensions are suspected, further study needed to confirm, and if these extensions are tidal tails or extended stellar halos. Overall, the galaxy appears to be a relatively quiescent system, possibly in the process of or having completed its transition into a red and dead object.
