The galaxy appears to be a disk galaxy, observed at a moderate inclination. There is a noticeable bulge, although not overly prominent. A significant portion of the light appears to originate from regions outside the central bulge, suggesting ongoing star formation. There are some indications of possible minor disturbances in the galactic structure. It is likely that it is a galaxy of substantial mass, with active star formation occurring throughout. There appears to be a companion object in close proximity, which could be interacting with the main galaxy, potentially contributing to the disturbances observed.
