The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, suggesting a spheroidal component with an older stellar population, as evidenced by the yellowish-orange hue. The isophotes appear generally round, with only minor deviations from perfect circularity. A subtle extension or disturbance is visible on one side, possibly indicating a minor interaction or tidal feature. Overall, the galaxy appears relatively quiescent in terms of star formation activity, based on the lack of prominent blue regions indicative of young, massive stars.
