The galaxy presents as a somewhat rounded, diffuse object. Its light is dominated by redder wavelengths, with a concentrated, bright core exhibiting a yellowish-white hue. There appears to be a slight elongation or minor disturbance visible, suggesting a possible interaction or internal dynamic affecting its morphology. Fainter, bluer regions are suggested within the extended halo. The galaxy lacks the distinct spiral arm features or a well-defined disk, indicating a possible early-type or spheroidal morphology. The overall structure suggests a system undergoing active star formation, despite its redder color, with the possibility of a recent or ongoing merger event contributing to its irregular shape and elevated star formation rate.
