The galaxy appears as a moderately bright, smooth object with a slightly elliptical morphology. The light distribution suggests a concentrated central bulge, which dominates the overall luminosity. The color gradient indicates a potentially aging stellar population. Redder hues are observed towards the outer regions, while the central region exhibits a bluer color, possibly indicating the presence of some active star formation. There are no obvious spiral arms, bars, or tidal features, leading to a classification of a relatively undisturbed galaxy. There is some slight asymmetry in the galaxy's overall shape and light distribution, although it does not present any obvious signs of a major ongoing merger.
