The galaxy presents as a centrally concentrated, smooth object with a slightly elongated, elliptical morphology. The core exhibits a bright, concentrated luminosity, indicating a high stellar density. Moving outwards from the core, the luminosity decreases gradually, with no distinct breaks or features suggesting spiral arms or a disk structure. The color profile appears relatively uniform across the galaxy, with a slight reddish-yellow hue, hinting at an older stellar population. There is a very minor perturbation on one edge of the galaxy, but otherwise the overall structure appears regular and undisturbed. The galaxy appears relatively isolated, lacking any obvious tidal features or nearby companions that would suggest recent interactions or mergers.
