The galaxy presents as a somewhat diffuse object, lacking a sharply defined nucleus. The overall morphology appears to be disturbed, with features suggesting a possible ongoing or recent merger event. There is evidence of tidal tails or extended structures, indicating gravitational interaction with another galaxy or galaxies. The color profile displays a range of colors across the visible spectrum. Regions of bluer hues may indicate younger stellar populations and active star formation, while redder regions may represent older stellar populations. The galaxy is of intermediate size, roughly 6.5 kpc across based on the provided measurements. There is no distinct spiral arm structure.
