The galaxy presents as a singular, largely spheroidal object. The light profile appears relatively smooth, with a concentrated central region. The primary color is a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. There is a slight bluer tinge that could indicate some younger, hotter stars are present, but the overall color suggests the galaxy is not dominated by recent or ongoing starburst activity. No spiral arms, bar structures, or prominent dust lanes are discernible. There is no evident tidal distortion or signs of an ongoing merger with another galaxy, and the morphology appears generally relaxed. Overall the galaxy appears to be of an elliptical classification.
