The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated luminosity profile, appearing nearly circular. There is a notable lack of discernible spiral arm structures or bar features. The galaxy is dominated by a yellowish hue, suggesting an older stellar population with a lower rate of star formation. No significant tidal tails or evidence of ongoing major mergers are apparent, although there might be minor asymmetry within the outer isophotes that could indicate a past interaction or minor disturbance. The color gradients across the galaxy appear subtle, with a slight reddening towards the core. The light is relatively concentrated, with the majority of the galaxy's light emitting from within a central radius of roughly 2 arcseconds.
