The galaxy presents as a smooth, centrally concentrated object, likely an elliptical galaxy. The core exhibits a bright, yellowish-white luminosity, suggesting a population of older stars. The light intensity decreases gradually outwards. The galaxy appears somewhat elongated, but not extremely so. There is a suggestion of faint, diffuse outer regions, which are difficult to resolve. Overall, the galaxy exhibits a lack of discernible features such as spiral arms or dust lanes. It is likely a galaxy which is not forming many new stars. The galaxy does not seem to be undergoing any major merging activity, as there is no evidence of strong tidal tails or other disturbances in its morphology.
