The galaxy presents as a somewhat elongated, lenticular structure, displaying a smooth, largely featureless morphology. The central bulge appears prominent and exhibits a bright, diffuse glow, indicating a significant concentration of stars. The color gradient across the galaxy suggests a possible variation in stellar populations, with the core potentially harboring older, redder stars, while the outer regions show hints of bluer hues, possibly indicating more recent star formation. There is a slight asymmetry in the distribution of light, and a small area of slightly elevated blue light to the side of the main galaxy body, hinting at a possible minor interaction or internal disturbance. The overall structure appears relatively undisturbed, suggesting that if any merger event occurred, it was either in the distant past, or a very minor interaction.
