The galaxy presents an overall elliptical morphology. Its core region is a bright, concentrated source of light, appearing yellowish, suggestive of an older stellar population. Fainter, bluer features extending from the central region may indicate some level of disk structure or recent star formation, although it is not well defined. A dust lane or some other obscuring structure is possibly present, causing an irregularity in the overall smoothness of the galactic disk. There is a mild disturbance in the galaxy's disk, either due to interactions with other galaxies or internal forces. Overall, the galaxy is moderately luminous, with hints of ongoing, but likely subdued, star formation activity.
