The galaxy presents a generally smooth morphology, with a slight elongation suggestive of a disk-like structure viewed at an angle. The central region displays a concentrated, bright yellowish hue, indicative of an older stellar population likely residing within the bulge. Progressing outwards, the colour shifts to a more bluish-white, indicative of younger stars within the disk. The galaxy's disk appears relatively undisturbed, with only minor indications of asymmetrical features or tidal disturbances. Overall, this galaxy shows characteristics intermediate between elliptical and spiral galaxies, with signs of star formation. 
