The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless with a centrally concentrated bulge that is approximately 8 kpc in effective radius. The isophotes appear to be moderately elliptical in shape, with a minor degree of asymmetry that could indicate a minor disturbance or interaction, though no clear tidal features are visible. The central region displays a yellowish-orange hue, suggestive of an older stellar population. Fainter, bluer regions are observable further out from the center. The light distribution is relatively smooth, with no prominent dust lanes or spiral arm structures immediately apparent. The overall color profile suggests a galaxy undergoing moderate star formation activity with an estimated stellar mass of approximately 10^10.9 solar masses.
