The galaxy presents a generally smooth, elliptical morphology with a slight elongation. A dominant central bulge is visible, exhibiting a yellowish-orange hue, which suggests a population of older stars. The overall color gradient indicates a potential lack of significant ongoing star formation, which is typical for galaxies with this morphology. There is a potential faint disk with hints of bluer regions toward the outer edges that suggests a minor amount of recent or current star formation, but it could also be due to background interference. There is no strong evidence of spiral arm structure, nor any clear signs of ongoing major mergers or tidal disturbances, though a slight asymmetry could indicate past minor interactions or accretion events. The galaxy is located at a significant distance, which limits detailed analysis of smaller features.
