The galaxy presents as a moderately bright, elliptical-like structure with a smooth light distribution. It is elongated, with the major axis appearing at an angle relative to the image frame. The central region is noticeably brighter than the outer regions, suggesting a concentration of older stellar populations. The galaxy exhibits a yellowish-white hue, indicative of a relatively evolved stellar population with lower rates of ongoing star formation. Faint, extended halos are marginally visible. There is no clear evidence of spiral arm structure or prominent dust lanes.
