The galaxy presents as a somewhat elongated, disk-like structure. A central bulge is visible, appearing relatively smooth and concentrated. The outer regions of the galaxy appear less defined, with a diffuse halo of fainter light extending outwards. The galaxy exhibits a blue hue, suggesting the presence of younger, hotter stars and ongoing star formation activity, potentially at a moderate rate. The overall morphology leans towards an intermediate type, displaying characteristics of both spiral and lenticular galaxies. There are hints of possible minor disturbances or asymmetries in the galaxy's structure, though no distinct tidal tails or major merger signatures are apparent. The elongated shape is visible, it can be seen that the roundness of the galaxy is somewhere in between a circle and cigar shaped.
