The galaxy presents as a centrally concentrated object with an overall bluish hue. The central region exhibits a brighter, compact core, surrounded by a more diffuse halo. The morphology appears somewhat irregular, hinting at potential gravitational interactions or internal disturbances. The outer edges of the halo appear elongated and slightly disturbed, with subtle evidence of tidal features or faint, extended arms. Redder regions are visible in the inner regions, suggesting older stellar populations, while bluer regions in the outer parts may indicate ongoing star formation. The general shape deviates noticeably from a perfectly elliptical or spiral form, indicating a more complex structure.
