This galaxy presents a somewhat irregular morphology, potentially exhibiting features of both spiral and elliptical types. A central, bright core region dominates, appearing nearly spherical and suggestive of a bulge component. Fainter, diffuse emission extends outwards from this core, with hints of a disk-like structure. The light distribution is not perfectly smooth, possibly indicating ongoing or recent interactions. There may be some dust lanes or regions of active star formation scattered within the disk, judging from the mottled texture and variations in color. The overall color appears to be a slightly blue hue, which would suggest a intermediate population of stars. Further spectral analysis would be necessary to confirm the age and metallicity of the stellar populations.
