The galaxy presents as a moderately luminous object, exhibiting a disturbed morphology possibly indicative of an ongoing or recent interaction. The primary body of the galaxy displays a somewhat irregular shape with a slight elongation, suggesting a non-relaxed structure. A brighter, more concentrated region is observed towards what could be the galactic center, which appears to be slightly off-center relative to the overall galactic structure.

Several distinct color gradients are visible within the galaxy. The central region presents a yellowish hue, which may indicate a population of older stars. Surrounding this central region, areas of bluer light suggest the presence of younger, hotter stars and possibly ongoing star formation. There appears to be some low-level spiral arm structure. There is an indication of tidal features or extended debris, appearing as diffuse extensions, potentially the result of gravitational disruption.
