The galaxy appears relatively compact, exhibiting a core with a bright central region of intense luminosity. Surrounding the core is an area with a more diffuse, albeit structured, distribution of light. Distinct features include potential regions of active star formation, indicated by somewhat clumpy areas with a greenish hue around the core. These regions are irregular and suggest a potentially ongoing interaction or internal disturbances. There is a faint, asymmetrical tail-like extension visible on one side, potentially indicating a minor tidal disturbance or interaction. The galaxy generally lacks the well-defined spiral arms usually associated with disk galaxies. The morphology appears more irregular than smooth, with noticeable texture around its edges, suggesting a disturbed system. The color profile appears to be dominated by greenish hues, possibly indicating a high rate of star formation.
