The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape approximates a slightly elongated ellipse. The color profile indicates a dominant population of older stars, evident in the reddish-yellow hue concentrated toward the core. A bluer, more diffuse component surrounds the central region, suggesting the presence of a younger stellar population or ongoing star formation, although the distribution appears uneven, with hints of patchiness rather than well-defined spiral arms. There is evidence of minor gravitational disturbance based on the distorted light to one side of the galaxy's central bulge. There are no tidal tails or clear signs of a major merger event currently in progress. Based on its appearance, it is likely an elliptical galaxy, but could also be a spiral galaxy that is viewed at a slight angle. 
