The galaxy presents as a somewhat diffuse structure with a discernible, albeit disturbed morphology. It exhibits a complex arrangement of light distribution, suggesting ongoing or recent interaction or internal dynamic processes. Two main concentrations of light are observed; one being dimmer than the other. Possible tidal tails or minor disturbances are visible along the left side of the galaxy. These features indicate possible gravitational interactions with another galaxy, or that these are clumpy regions of star formation. The colours range from slightly reddish in certain regions to bluish. The relatively brighter, bluish regions may indicate areas of active star formation containing younger, hotter stars. The reddish areas may indicate older stellar populations or dust lanes. The overall shape isn't well defined, leaning neither toward purely elliptical nor spiral, but the light concentrations suggest a somewhat irregular shape. Further analysis, including spectroscopic data, is needed to determine the nature of the interaction.
