The galaxy presents a largely featureless, smooth appearance, suggestive of an elliptical or lenticular morphology. It exhibits a concentrated central bulge, appearing almost spherical, with a gradual decrease in luminosity moving outwards. The color is generally consistent, with a yellowish-orange hue across the visible spectrum. Faint, diffuse extensions are potentially present, but subtle. Based on the color profile, it appears to be composed of an older stellar population, with lower levels of star formation. Minor disturbances are observable, indicating a possible history of minor interactions with other galactic objects. This galaxy is not actively undergoing a major merger.
