The galaxy presents as a slightly inclined disk, exhibiting a predominantly bluish hue, suggestive of ongoing or recent star formation activity. Patches of more intense blue concentrations are visible, likely representing regions of heightened star formation, potentially starburst regions or clusters of young, hot stars. The overall morphology hints at some level of disturbance or interaction. While a defined spiral structure is not readily apparent, there seems to be a hint of asymmetric distribution of light, which may suggest some tidal interaction. The galaxy appears moderately luminous. The light is relatively smooth, but still clumpy, across its extent. The redder galactic bulge is smaller than the galactic disk. The galaxy's color is suggestive of a population of young stars.
