The galaxy presents as a relatively bright object with a smooth, centrally concentrated luminosity profile. It exhibits a somewhat elliptical shape, appearing nearly round, although subtle elongation is present. The core region shows a whitish-yellow hue, suggesting a concentration of older stellar populations. Moving outwards, the light becomes bluer, possibly indicating the presence of younger stars and ongoing star formation within the galactic disk. There is no strong evidence of spiral arm structures or other pronounced features. The outer edges appear diffuse, gradually fading into the background. There is a faint possibility of minor tidal disturbances or interactions, but without higher resolution, it's hard to confirm if the asymmetry is due to noise or a physical phenomena.
