The galaxy appears as a centrally concentrated, roughly elliptical object. The core exhibits a bright, yellowish-white hue, suggesting a high density of older stellar populations. Moving outward from the core, the color transitions to a dimmer, greenish-blue tinged halo. This may indicate a more dispersed population of stars, or the presence of some star forming regions. The overall structure appears relatively smooth with no prominent spiral arm structure. There are no signs of strong tidal disturbances, major asymmetries, or close companion galaxies suggesting any recent major merger events. The overall shape is more "in between" than perfectly round or cigar shaped.
