The galaxy presents as an inclined spiral or a disk galaxy, viewed at an oblique angle relative to its plane. A prominent central bulge is visible, exhibiting a concentrated luminosity, appearing yellowish in color. Fainter disk structures extend outwards from the bulge, with some indications of arm-like features, but lacking clear definition. The disk appears somewhat asymmetric, suggesting possible interactions or internal disturbances. The overall color profile implies a mix of stellar populations, the yellowish hue of the central bulge potentially indicating older, redder stars, while the disk exhibits hints of bluer regions that could represent younger, star-forming regions. There is a presence of what looks like a smaller galaxy that it might be interacting with. The galaxy's morphology suggests it could be undergoing some form of evolutionary transition, with the blurring of structures indicative of ongoing processes that will define its morphology.
