The galaxy appears as a somewhat elliptical, centrally concentrated object. It exhibits a smooth, diffuse morphology, with no prominent spiral arms or distinct features immediately apparent. The color profile indicates a dominant yellowish-orange hue in the central bulge region, possibly indicative of an older stellar population. Fainter, bluish-white light is present in the outer regions of the galaxy, which could point to the presence of a younger, hotter population of stars. There is some irregularity of the shape in the outskirts, suggesting a possible minor interaction or disturbance.
