The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. There is little to no evidence of spiral arms or a distinct disk structure. The central bulge is prominent and appears relatively bright, suggesting a concentration of older stellar populations. The galaxy displays a color gradient, with the core exhibiting a yellowish-orange hue, indicative of evolved stars. Moving outward from the core, the color shifts slightly towards redder tones, possibly due to the presence of dust or a different population of older stars. There is no evidence of strong star formation activity. A small fraction of mergers or disturbances are present. The galaxy seems relatively isolated and undisturbed, with a regular overall structure.
