The galaxy presents as a flattened, disk-like structure with an overall smooth appearance. It exhibits a yellowish hue, suggesting a stellar population dominated by older, cooler stars. There is a central bulge region that appears brighter and more concentrated than the surrounding disk. The galaxy's shape is somewhat elongated, leaning towards a cigar-shaped morphology, and no prominent spiral arms are discernible. There are no signs of any major disturbances or ongoing mergers. Overall, the galaxy seems to be relatively quiescent, showing little evidence of recent or intense star formation.
