The galaxy presents as a somewhat elliptical, disc-like structure, with the disk oriented at an angle relative to our line of sight. The central region exhibits a bright, concentrated bulge, appearing yellowish-white in color. This suggests a population of older stars. Moving outward from the bulge, the disk becomes more diffuse and less luminous, with a general blueish-white color. This indicates younger stars and possibly ongoing star formation. There are some very faint hints of spiral arms extending outward, but they lack clear definition. There is no evidence of any major mergers or significant tidal disturbances affecting the galaxy's overall morphology. The galaxy appears relatively isolated and undisturbed.
