The galaxy presents a largely featureless morphology, appearing primarily smooth and elliptical in shape. It displays a concentration of light towards the center, suggesting a prominent bulge component. The outer regions exhibit a gradual decrease in luminosity, fading into the background sky. The color profile indicates a predominantly older stellar population, with a yellowish-red hue. There is no apparent spiral structure or significant dust lanes visible in this image, though higher resolution images and analysis are required for a more precise characterization of the galaxy's detailed structure and internal dynamics. No immediate signs of major mergers or tidal disturbances are evident, though there appears to be a potential minor disturbance in the galaxys morphology. This is indicated by a slight change in brightness on the lower half of the galaxy.
