The galaxy presents as a slightly elongated, elliptical-like structure. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars in the central region. A diffuse halo surrounds the core, fading in intensity outwards. The overall color appears yellowish-white in the center, possibly indicating an older stellar population. Fainter, blueish regions are observable within the outer portions of the disk and the edges of the galaxy, which may indicate pockets of ongoing star formation. There may be minor gravitational disturbance or a merging event occurring, however there are no significant visual signs of a major collision or disruption to the overall galactic structure.
