The galaxy presents as a somewhat diffuse, amorphous structure, exhibiting a generally smooth appearance with a slight elongation. Its core region is characterized by a brighter concentration of light, suggesting a higher density of stars. There is little evidence of spiral arm structure. The galaxy displays a dominant blue hue, particularly pronounced in the central region, possibly indicating ongoing star formation. Patches of less distinct redder components are scattered across the galaxy, implying the presence of older stellar populations. The overall structure suggests a relatively undisturbed system, lacking significant tidal features or strong asymmetries usually associated with major mergers. However, there may be hints of subtle disturbances or minor interactions, warranting further investigation. The galaxy is likely a low-mass system, with a moderate rate of ongoing star formation.
