The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a relatively smooth light distribution, with a dominant bulge component visible in the core. There may be faint hints of a disk-like structure, but it is not well-defined, with no easily distinguishable spiral arms. The galaxy appears to be slightly disturbed, possibly due to a minor interaction with another galaxy or a recent merger event. It displays a yellowish-reddish hue, suggesting a population of older stars and low ongoing star formation. Based on morphology and color, this galaxy may be an early-type galaxy at an intermediate redshift.
