The galaxy presents a morphology suggestive of an elliptical galaxy, exhibiting a largely featureless and smooth appearance. Its overall shape is elongated, though only modestly so. There is no obvious structure, such as spiral arms or a prominent disk. The central region appears brighter and more concentrated, indicative of a higher stellar density typical of galactic bulges. The color profile is relatively uniform throughout the galaxy, showing a tendency towards reddish hues, possibly indicating an older stellar population and lower ongoing star formation activity. Subtle irregular features may point towards a past interaction or minor disturbance. The galaxy is relatively compact.
