The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile suggests a concentrated central bulge, with a gradual decrease in luminosity moving outward. The galaxy exhibits a yellowish-orange hue, potentially indicative of an older stellar population with reduced recent star formation. There is no discernible spiral arm structure or prominent dust lanes visible in this image. The galaxy's overall morphology appears largely undisturbed, although very subtle irregularities in its outer regions may suggest minor gravitational interactions or past merger events.
