The galaxy presents as a centrally concentrated, elliptical system. The core exhibits a smooth, high-surface-brightness profile with a color gradient shifting towards redder hues in the innermost regions. Progressing outwards from the nucleus, the galaxy displays a broader, less concentrated halo characterized by a gradual decrease in surface brightness. There is some evidence of a slightly elongated morphology, possibly hinting at a mild triaxial shape. Overall, the galaxy lacks prominent spiral arms or distinct features indicative of active star formation. The color profile suggests a relatively old stellar population, though there are hints of younger stars residing in the outer disk. There is no apparent strong interaction with neighboring galaxies, and its morphological features seem largely undisturbed.
