The galaxy presents as an elongated, disk-like structure, suggesting a spiral or lenticular classification, viewed at a high inclination. The central bulge appears relatively prominent and exhibits a yellowish hue, potentially indicating a population of older, redder stars. Fainter, bluish regions are visible within the disk, possibly representing areas of more recent star formation. There is no clear evidence of strong spiral arm structure or major disturbances, although a slight asymmetry in the outer regions might suggest minor tidal interactions. The galaxy appears moderately distant, and its colors indicate the light has been significantly redshifted. Overall, it seems like a galaxy of intermediate mass, with modest levels of ongoing star formation.
