The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape appears elliptical, elongated slightly with a cigar-like appearance. There are no immediately discernible spiral arms or distinct features, suggesting it is most likely an elliptical galaxy. The core exhibits a bright, yellowish hue, likely indicative of an older stellar population. The outer regions show a gradual decrease in brightness, with a color gradient shifting towards a redder tint. This color variation may reflect differences in stellar population and age distribution, with older, redder stars dominating the outer regions. No signs of ongoing major mergers or significant tidal disturbances are observed.
