The galaxy presents a relatively smooth, elliptical morphology with a highly concentrated central bulge. The light profile appears largely uniform, lacking distinct spiral arm structures or prominent star-forming regions. The color index indicates a population of older stars, emitting strongly in the redder bands. There is a subtle asymmetry to the overall shape, possibly indicative of a minor interaction or internal disturbance, although no clear signs of a major merger are evident. The galaxy exhibits a compact size with a high degree of roundness and a lack of observable tidal features or extended halos. Overall, the galaxy appears to be a well-formed, evolved system, likely a massive elliptical galaxy.
