The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge that appears yellowish-white, suggesting an older stellar population dominating the core. The overall shape is elongated, with an axis ratio indicating a flattened structure. A faint, diffuse disk is suspected, but there is minimal evidence of spiral arm structure. The color gradient indicates a bluer outer region, hinting at the presence of some younger stars or ongoing star formation in the galaxy's periphery. A subtle asymmetry in the light distribution may indicate a minor disturbance or possible merger event in the galaxy's past.
