The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge that dominates the overall structure. The outer regions exhibit a gradual decrease in surface brightness, fading into the background sky. The color profile indicates a relatively older stellar population, with a yellowish hue in the central region, suggesting a prevalence of evolved stars. There is some evidence of a faint disk-like structure, appearing as a flattened distribution of light surrounding the core. No distinct spiral arms or dust lanes are visible. The overall appearance suggests the galaxy is in a relatively quiescent state, with limited ongoing star formation activity. There is no visual evidence of any major mergers or significant tidal disturbances.
