This galaxy presents as a somewhat elongated structure, potentially disk-like, viewed at an inclined angle relative to our line of sight. The central region exhibits a concentration of light, likely indicating a bulge or core component. The color profile suggests the presence of both older stellar populations, indicated by reddish hues in the core, and possibly younger, bluer stellar populations in the surrounding disk. There is a faint, diffuse halo around the bright center of the galaxy. The apparent shape and structure suggest that the galaxy may have undergone some minor disturbances, potentially due to previous gravitational interactions or internal processes. There is no clear evidence of active merging.
