The galaxy presents a concentrated, elliptical morphology. Its color profile suggests a population of older stars, exhibiting a yellowish hue, with minimal evidence of active star formation. The core is relatively bright and well-defined, gradually fading into the surrounding halo. There is a smooth, featureless appearance dominating the structure of the galaxy. The shape is between round and elliptical, with no apparent spiral arms, bars, or other distinct features characteristic of disk galaxies. There is no indication of major mergers or tidal disturbances that might disrupt its smooth structure.
