The galaxy presents a smooth, elliptical morphology, appearing largely featureless at this resolution. It exhibits a concentrated central bulge with a gradual decrease in luminosity outward. The color profile suggests a relatively evolved stellar population, dominated by older, redder stars. No distinct spiral arms or prominent dust lanes are discernible. There is no apparent major distortion in the galaxy's structure, hinting to a quiescent state without ongoing major mergers. Faint indications of a minor interaction or disturbance are plausible, though not definitively evident in the imagery. Overall, the galaxy presents as a well-formed elliptical galaxy with a relatively homogenous structure.
