The galaxy presents as a somewhat elliptical structure, appearing mostly smooth in texture without distinct spiral arms or bar features. There is a gradual increase in luminosity towards the central region of the galaxy, suggesting a concentrated nucleus. The overall color appears to be a yellow-orange hue, which may indicate a population of older stars, or a moderate amount of dust obscuration. Slight elongation is visible, with a deviation from a perfectly circular morphology. No significant tidal tails or signs of major mergers are readily apparent.
