The galaxy presents as a concentrated, ellipsoidal structure, indicative of an elliptical or lenticular morphology. Its central region exhibits a high degree of luminosity, suggesting a dense stellar population or possible AGN activity. The light profile gradually decreases from the core outwards, with a smooth transition to the outer regions. There are no discernible spiral arms or prominent dust lanes visible in this image, supporting the classification of a relatively featureless, evolved system. The color appears slightly redder, which indicates an older stellar population and suppressed star formation activity, which appears to be low. There is no indication of strong tidal disturbances or ongoing merger events. The galaxy is relatively isolated.
