This galaxy appears to be an elliptical type, exhibiting a smooth, generally featureless morphology. The light distribution suggests an elongated, cigar-like shape, with a brighter central region and a gradual decrease in luminosity outwards. There is no discernable spiral structure or dust lane. The color gradient indicates a central bulge that appears more yellow/orange, suggesting an older stellar population. The outer regions display a slight bluer tint implying more active, but subdued, star formation. There is no obvious evidence of a major ongoing merger, although a minor disturbance or interaction cannot be completely ruled out based on the subtle asymmetry observed in its outer regions.