The galaxy presents as an elongated, elliptical form with a smooth, diffuse light distribution. There is a concentration of luminosity towards the central region. The outer regions exhibit a gradual fading in intensity, suggesting a lack of distinct spiral arm structures. The color gradient transitions from a yellowish-white core, potentially indicative of an older stellar population, to a bluer hue in the outer regions. The pronounced ellipticity may imply that it is seen at a large angle relative to its plane of rotation. There is no clear evidence of a bulge or spiral structure. Overall, it appears as a relatively quiescent galaxy.
