The galaxy presents a generally smooth and elliptical morphology. Its core exhibits a concentrated, bright luminosity, appearing yellow-white in color, suggesting a population of older stars. Moving outward from the center, the light diffuses gradually into a less luminous halo with a blueish tinge. There are no clearly discernible spiral arms or bar structures visible. The object appears mostly undisturbed, with no obvious signs of ongoing major mergers or tidal distortions in its outer regions. The overall color profile indicates a evolved stellar population. Its elongated shape suggests it may be an elliptical galaxy, or a spiral galaxy viewed at an angle.
