The galaxy presents as a moderately luminous object with a noticeable elliptical morphology. The central bulge is a dominant feature, exhibiting a smooth, concentrated distribution of light, indicating a high density of older stellar populations. The color of the bulge appears to be predominantly yellow-red, suggestive of a significant population of evolved, cooler stars.

A fainter, more diffuse disk component is visible surrounding the central bulge. The transition from the bulge to the disk is relatively smooth, lacking prominent spiral arm structures. The disk appears less concentrated than the bulge, with a bluer color, hinting at the presence of younger stars and ongoing, albeit low-level, star formation activity. 

There are subtle indications of minor disturbances or asymmetries in the outer regions of the galaxy, potentially suggesting a past interaction or merger event. The overall structure appears relatively undisturbed, suggesting that any interactions were likely minor. The galaxy does not appear to be undergoing a major merger or exhibiting strong tidal features.
