The galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge that emits strongly, indicating a high stellar density. Moving outwards from the center, the light gradually diffuses, with no distinct spiral arm structures or prominent dust lanes visible. The overall shape is moderately rounded, and the galaxy appears undisturbed, showing no significant signs of tidal distortions or ongoing mergers. The galaxy is yellowish-white suggesting an older stellar population and relatively low ongoing star formation.
