The galaxy presents as a spiral type, seen nearly face-on. Two spiral arms are clearly visible, winding outwards from a slightly brighter, condensed central bulge region. These arms exhibit a patchy structure, suggesting active regions of star formation. The color distribution across the galaxy indicates a possible gradient in stellar populations, with bluer hues dominating the spiral arms, consistent with younger stars and ongoing star formation. The central bulge appears somewhat redder, which could indicate an older stellar population. The overall structure appears slightly disturbed, possibly due to minor gravitational interactions or internal dynamics. The galaxy has a moderate size. There is no sign of a bar structure.
