The galaxy presents an elongated, disk-like structure with a clearly defined central bulge. The bulge appears relatively bright and concentrated, suggesting a significant stellar population. Moving outwards from the center, the disk exhibits a bluer hue, indicative of more recent or ongoing star formation within its spiral arms. The edges of the galaxy's disk appear somewhat irregular, possibly indicating tidal interactions or recent merger events. Though somewhat smooth in appearance, hints of spiral structure can be discerned. The overall morphology leans towards a disk galaxy seen at an inclined angle. Evidence for any major disturbances or ongoing mergers is subtle but some minor disturbances may be affecting its current morphology.
