The galaxy presents as a well-defined, elongated elliptical shape. The core region exhibits a concentrated, bright luminosity, appearing smooth and relatively featureless in this image. The light distribution suggests a centrally concentrated stellar population, likely dominated by older stars. Progressing outward from the core, the light gradually diminishes, with a smooth transition into the surrounding background. Some faint, diffuse bluer regions appear at the edge of the galaxy, possibly indicating some more recent star formation. No prominent dust lanes or spiral arm structures are discernible. The overall appearance is consistent with a galaxy undergoing little to no major disturbances or mergers.
