The galaxy appears to be an elliptical or lenticular type, characterized by a relatively smooth and featureless structure. Its shape is moderately elongated, leaning more toward a rounded form than a highly elongated cigar shape. The central region exhibits a concentrated luminosity, suggesting a significant stellar population density, while the outer regions display a gradual decrease in brightness. The galaxy's color gradient indicates a possible mix of stellar populations, with a yellowish hue concentrated towards the center and a bluer tint in the surrounding areas. There are subtle asymmetries, hinting at possible minor gravitational interactions with other galaxies. Overall, the galaxy appears to be a relatively isolated system, without prominent indications of ongoing major merger activity.
