The galaxy presents as a generally smooth, elliptical morphology. Its central region exhibits a bright, concentrated luminosity, suggesting a high stellar density and possibly an active galactic nucleus. The color is primarily yellow-orange, indicating a population of older stars with lower rates of recent star formation. There is a notable lack of discernible spiral arms or prominent dust lanes. The overall structure appears undisturbed, showing no signs of major mergers or tidal interactions. The shape is somewhat elongated, deviating slightly from a perfectly circular form.
