The galaxy presents as a slightly irregular, disk-dominated morphology, with some evidence of internal structure beyond a purely elliptical profile. A central bulge is visually discernible, exhibiting a higher surface brightness than the surrounding disk. The disk shows a non-uniform color distribution, with some regions appearing bluer, potentially indicating areas of more recent star formation. There seems to be a slight asymmetrical disturbance to the outer part of the galaxy, which may be attributed to a minor interaction. Overall, the galaxy exhibits properties consistent with a moderate-mass, actively star-forming system.
