The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its form approximates a circular shape, exhibiting a high degree of roundness. There is no evident disk structure or spiral arm features. The galaxy exhibits a color gradient, with a more pronounced yellow/orange hue toward the central region, possibly indicating an older stellar population in the core. The outer regions display a slightly bluer tint, suggesting the presence of some younger stars, though star formation appears limited. No signs of ongoing major mergers or significant tidal disturbances are visible. The galaxy seems to exist in relative isolation within the observed field. Overall, the galaxy appears to be a relatively evolved system.
