The galaxy presents a complex morphology, exhibiting characteristics of both spiral and elliptical galaxies. A notable feature is the prominent bulge region, which, while not fully dominant, constitutes a substantial portion of the galaxy's overall structure. The disk component appears to be significantly inclined relative to the line of sight, tending towards an edge-on orientation. There is evidence suggesting the presence of spiral arms, though they are not sharply defined, indicating a possible flocculent structure. The presence of a central bar feature is also noticeable, yet its classification is uncertain, being somewhere between a weak and non-existent bar structure. There are signs of disturbances to the galaxy's structure, suggesting possible interactions or past mergers. Additionally, the light from the galaxy reveals moderate star formation activity.
