The galaxy presents a relatively smooth, elliptical morphology. It appears nearly circular, with a slight elongation noticeable in its overall shape. The central region exhibits a high concentration of light, suggesting a prominent bulge. The colour gradient indicates an older stellar population, with a redder hue in the core transitioning to a bluer tinge in the outer regions. This colour difference potentially suggests ongoing, but low, levels of star formation in the galaxy's outskirts. No distinct spiral arms or prominent dust lanes are visible within the galaxy's structure, further supporting its classification as an elliptical type. There is a slight asymmetry in the light distribution, hinting at a potential minor interaction or disturbance in its past. Overall, the galaxy appears to be a massive system, with little recent star formation and a mature stellar population.
