The galaxy presents as a moderately luminous object with a discernible, though not highly pronounced, disk-like structure. The central bulge appears relatively prominent and exhibits a yellowish hue, suggesting a population of older, redder stars. Moving outward from the core, the disk displays a bluer coloration, indicative of ongoing star formation and a younger stellar population. There's a slight indication of irregularities or faint features within the disk, possibly hinting at minor disturbances or interactions. The galaxy's overall shape deviates slightly from perfect circularity; it exhibits a somewhat elongated morphology. There is no clear indication of any major merging events and the galaxy seems to be relatively isolated.