The galaxy presents a largely smooth and rounded appearance, suggesting an elliptical morphology. The central region exhibits a concentrated luminosity, fading gradually towards the outer edges. Faint hints of blue can be observed along the periphery, intermixed with redder tones, which may indicate regions of ongoing star formation, albeit at a low rate relative to its overall mass. There is no discernable spiral arm structure or prominent dust lanes, further supporting an elliptical classification. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
