The galaxy presents as a slightly elliptical, moderately concentrated light source. The dominant color appears to be a blue-green hue, potentially indicating recent or ongoing star formation. A fainter, more diffuse region is visible adjacent to the central part of the galaxy, with a color gradient suggesting older stellar populations or dust obscuration. Overall, there does not appear to be any signs of spiral arms, making it appear relatively smooth. There is no distinct tidal tail or indications of major mergers; however, there may be evidence of slight asymmetry.