The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse, extended halo. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features indicative of active star formation regions. The color profile suggests a population of older stars, with a redder hue in the central regions gradually fading towards the outer edges. There is no evidence of significant tidal interactions or ongoing merger activity. The overall structure appears relaxed and well-defined, consistent with a mature elliptical galaxy.
