The galaxy presents a generally smooth morphology, exhibiting characteristics of an elliptical galaxy. It appears largely featureless, with no prominent spiral arms or distinct structures discernible in the image. The galaxy's light profile suggests a spheroidal shape, elongated in a slight cigar-like fashion, with the light intensity concentrated towards the central region, indicating the presence of a bright galactic nucleus. The colour gradient transitions smoothly from a yellowish-white core to a redder outer halo. This color distribution suggests a population of older stars dominates the galaxy, while the core includes relatively young stars. Evidences suggest that the galaxy does not show any signs of recent major mergers or significant disturbances.
