The galaxy presents a morphology that is somewhere between smooth and featured. Its apparent shape is elongated, trending towards cigar-shaped rather than perfectly round. A significant fraction of classifications suggest a merging event.

The color distribution within the galaxy is not uniform. The central region exhibits a more yellow hue, which could indicate an older stellar population. A fainter, bluer component is observed extending outward from the central region. This suggests ongoing or recent star formation activity. The spatial distribution of the blue component is not entirely uniform.

There are signs of disturbances in the galaxy's structure. The overall shape is asymmetrical. These features suggest potential interactions with other galaxies or internal dynamic processes influencing its overall appearance and star formation rate.
