The galaxy presents as a somewhat diffuse object with a central region of increased luminosity, indicative of a galactic nucleus. The overall morphology suggests the potential presence of a disk structure, though it is not sharply defined. There are subtle asymmetries in the distribution of light, hinting at possible past interactions or internal disturbances. The galaxy exhibits a blue hue, which may imply recent or ongoing star formation activity. There does not appear to be a strong presence of dust lanes or distinct spiral arm structures. The outer edges of the galaxy fade gradually into the background, suggesting a relatively smooth density profile. Overall, the galaxy appears to be a low-mass system with moderate levels of star formation and possible morphological disturbances.
