This galaxy presents as a disk galaxy seen almost perfectly edge-on. The dust lane is not easily discernible, though the galaxy displays a flattening that implies a strong disk structure. The bulge is not particularly pronounced, appearing somewhat boxy. There appears to be some slight minor disturbances but is mostly undisturbed, displaying no obvious signs of a major merger. The overall color suggests a mix of stellar populations, with blue indicating a fraction of ongoing star formation alongside a population of redder, older stars. Considering its inferred size and luminosity, this galaxy is likely a dwarf galaxy.
