The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a high degree of luminosity, appearing bright yellow, indicative of an older stellar population. The overall shape can be described as somewhat elongated, exhibiting a cigar-like morphology. There appears to be a relatively smooth light distribution, showing little evidence of spiral arms or significant dust lanes. There is a slight hint of bluer regions on the outer edges of the galaxy, hinting at possible star formation. The shape is relatively undisturbed, with some signs of minor disturbance.
