This galaxy exhibits a disk-like morphology, inclined relative to our line of sight. The central region displays a brighter, more concentrated luminosity profile, suggestive of a galactic bulge. The disk component is not uniformly smooth, showing some features such as flocculent arms or irregular light distribution. There are subtle hints of blueish color in the disk, particularly towards the outer regions, which may indicate ongoing star formation. The overall structure appears somewhat disturbed, possibly due to a past or ongoing minor merger event, or internal dynamical processes. There does not appear to be any major merger in progress, although subtle distortions are visible. The galaxy has a moderate size and luminosity, potentially placing it in the range of a Milky Way analog.
