The galaxy presents a morphology consistent with a spiral type, observed at an inclined angle relative to our line of sight. The galactic disc is evident, exhibiting a notable flattening. Within the disk, spiral arm structures are discernible, although their definition is somewhat diffuse. A central bulge region is apparent, characterized by a relatively smooth and concentrated luminosity profile, yellowish in color. There is indication of a bar structure crossing the galactic center, although not strongly pronounced. The galaxy is of intermediate size. There are no obvious signs of a major ongoing merger event.
