The object appears to be a galaxy, likely an elliptical type, given its overall smooth and featureless morphology. There is no apparent spiral structure or disk-like appearance discernible in the image. The galaxy exhibits a concentrated central region that gradually diffuses outward, implying a spheroidal distribution of stars. A color gradient is also apparent; the central region has a yellowish or golden hue, while the outer regions exhibit a slightly more reddish color. This color variation could be caused by differing stellar populations and dust distribution within the galaxy.

Given the smooth morphology and color gradient, it is plausible that the stellar population in the central region is older and metal-rich compared to the outer regions. There is no evidence of any ongoing major merging activity or significant disturbances in its structure. The general roundness indicates that it is not a highly elongated elliptical, but closer to a spherical shape.
