The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated luminosity profile. A distinct, bright nucleus is observed, surrounded by a diffuse, less luminous halo. The halo appears relatively featureless, without prominent spiral arms or dust lanes visible in this image. The overall shape approximates a circular or elliptical form, displaying a high degree of roundness. There is no visually discernible evidence of ongoing major mergers or tidal disturbances affecting the system's structure. The galaxy's color suggests a relatively evolved stellar population.
