The galaxy presents as a somewhat lenticular or early-type spiral morphology, with a smooth, elliptical light distribution. A central bulge is visible, with decreasing luminosity outwards and a lack of discernable spiral arm structures. There appears to be very little active star formation present. The galaxy is observed to be slightly more luminous in redder wavelengths, with little color variation across the central region, indicating an older stellar population. There is no distinct dust lane or any signs of tidal disruption. The overall roundness is moderate. There are no obvious signs of any ongoing major or minor merging events. The observed redshift suggests the galaxy is a considerable distance away, with a corresponding estimated size of a dwarf or intermediate galaxy. The blue magnitude suggests relatively low levels of star formation. Overall, this galaxy appears to be a relatively quiescent system.
