The galaxy presents a moderately inclined disk-like structure. There appears to be a central bulge, exhibiting a brighter, concentrated luminosity. Faint spiral arm segments are potentially present, but indistinct; there are signs of disturbances. The overall color is predominantly blue with red patches which indicates there may be some areas of more intense recent star formation as well as old stars. The galaxy is estimated to be about 3.5 kpc in radius, although its disk may be slightly more extended. Evidence suggests the galaxy may be undergoing a merger or experiencing tidal interactions, indicated by the amorphous and irregular morphology. The light distribution suggests the stellar mass is around 10^9 solar masses. The blue color implies a relatively low star formation rate, resulting in specific star formation rate of 10^-9.6 per year.
