The galaxy presents as a relatively smooth, elliptical-like structure with a high degree of central concentration. The color profile suggests a population dominated by older stars, displaying a yellowish-orange hue throughout the galaxy body. There are no prominent spiral arms or obvious dust lanes visible. The overall shape appears largely spheroidal with no significant distortions or tidal features indicative of recent major mergers, although some subtle irregularities in the outer regions cannot be ruled out definitively. The galaxy exhibits a centrally bright core, and is quite compact with a estimated diameter around 3 kpc. Analysis suggests the stellar mass of this object is roughly 10^10 solar masses. Star formation activity is low within the galaxy.
