The galaxy presents as a complex, asymmetrical structure. The core region exhibits a concentrated luminosity with a yellow-orange hue. Moving outward from the core, a diffuse, less structured disk is suggested, although disturbed features are present, with a color gradient towards redder tones. There is evidence of possible minor disturbances or interactions, though no clear merging activity is visually apparent. Overall, the galaxy appears to be a disk galaxy with some irregularities in its structure and a moderate level of star formation.
