This galaxy presents as a somewhat irregular, disk-shaped structure, exhibiting a relatively small angular size on the sky. A bright, central region of high luminosity is clearly visible, potentially indicating a dense stellar population or an active galactic nucleus. The surrounding disk appears relatively smooth, lacking prominent spiral arm structures, although some subtle, diffuse features may be present. There is a hint of minor disturbances in the galactic structure that could be an indication of minor interactions with another galaxy. Overall, the galaxy exhibits a non-distinct morphology, not strongly elliptical, but with some disturbances.
