The galaxy presents as a moderately luminous, elongated object. Its overall morphology is smooth with some features that suggest it may be a spiral galaxy viewed at an angle. The central region is relatively bright, appearing almost spheroidal, suggesting a bulge component. Fainter, disk-like extensions are seen with hints of spiral structure. These are characterized by a bluer hue, particularly towards the outer edges, suggesting ongoing star formation. The overall color of the galaxy is slightly redder, indicating an older stellar population compared to the bluer, star-forming regions. There appears to be little sign of any significant merger activity or major disturbances to its morphology, though there is some irregularity to the outer edges of the disk, which may suggest interactions with smaller companion objects or internal dynamics.
