The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in intensity outward from the core. The central region shows a yellowish hue, suggestive of an older stellar population, while the outer regions appear subtly bluer, potentially indicating the presence of younger stars, though this is not definitive. There are no prominent spiral arms or distinct dust lanes visible. There appears to be minimal, if any, disruption in the galaxy's overall structure. This galaxy shows little evidence of ongoing or recent major mergers.
