The galaxy presents as a centrally concentrated, smooth object. It exhibits a largely elliptical morphology, appearing quite rounded in shape. The central region is bright, indicating a higher density of stars or potentially an active galactic nucleus. The light profile smoothly diminishes outwards from the center, lacking any discernible spiral arm structure or distinct features. The galaxy displays a subtle color gradient, shifting from a bluer-white core to a slightly redder halo. This suggests a central population of relatively young, hot stars, while the outer regions may be dominated by older, cooler stellar populations. There is no clear evidence of ongoing merging activity or tidal disturbances. The galaxy appears relatively isolated and undisturbed in the observed field.
