The galaxy presents a generally smooth morphology. The dominant light appears concentrated toward the central region, which exhibits a yellowish hue. This could indicate an older stellar population within the bulge. Extending outward from the central region, a fainter, bluish haze is observed, possibly representing a disk component with ongoing, though not vigorous, star formation. There is some evidence of a tidal tail extending from the upper portion of the disk. The overall shape appears somewhat irregular, with indications of a possible interaction or minor disturbance.
