This galaxy exhibits a generally smooth morphology with a discernible central bulge. There is evidence of a disk structure, but it appears disturbed. Overall, it appears to be in a state of interaction or merging with another galactic object. The central region displays a bright, yellow-orange hue, suggesting an older stellar population or significant dust obscuration. Faint bluish regions may indicate areas of recent star formation. The galaxy is moderately sized and relatively close, based on apparent brightness and color. The overall shape of the galaxy appears somewhat irregular, possibly indicating tidal effects from an ongoing interaction or recent merger.
