The galaxy presents as a centrally concentrated object with a generally smooth morphology, showing little evidence of spiral arms or prominent disk structures. Its overall color is predominantly yellowish-white, suggesting a population of older stars. The central region appears to be brighter, indicative of a concentrated stellar population or a possible active galactic nucleus, though no distinct features are apparent at this resolution. The galaxy exhibits a moderate ellipticity, appearing somewhat flattened. There is no obvious dust lane or other signs of significant obscuration within the galaxy. Slight disturbance or distortion is possible, but a relaxed state is most likely.
