The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. There is a bright, somewhat diffuse core, which gradually fades outwards. The color appears to be predominantly blue, suggesting the presence of relatively young, hot stars. There appears to be at least one or more major disturbances, possibly due to an ongoing or recent merger event. No distinct spiral arm structures are discernible. The galaxy is of intermediate size, not exhibiting properties of a dwarf galaxy, nor exceptionally large spiral galaxy. There's a notable lack of dust lanes or clearly defined HII regions. The overall impression is that of a transitioning system experiencing interaction-induced star formation.
