The galaxy appears to be an elliptical galaxy, characterized by its generally smooth and featureless morphology. It exhibits a high degree of central concentration of light, with the intensity gradually decreasing outwards from the core. The overall shape approximates a spheroid, displaying a round appearance with only minor deviations from perfect circularity. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy is predominantly yellowish-white in color, suggesting an older stellar population and a relatively low rate of ongoing star formation. There are no visible signs of major mergers or significant tidal disturbances affecting the galaxy's structure, implying that it has likely undergone a relatively quiescent evolutionary history. Faint outer regions suggest a substantial but diffuse halo extending beyond the more concentrated central regions.
