The galaxy presents as a centrally concentrated, elliptical-like structure. The core exhibits a bright, golden-yellow hue, suggesting a population of older stars. Moving outward from the core, the color gradually transitions to a redder tone. The galaxy appears relatively smooth in texture with no distinct spiral arm features. There is no obvious indication of ongoing major merging activity or significant tidal disturbances, although subtle minor disturbances cannot be ruled out. The galaxy's overall morphology suggests an evolved system, likely with a high stellar mass and a relatively low specific star formation rate. The shape tends towards elliptical, as opposed to a well-defined spiral disk.
