The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a radial gradient, with a bright, concentrated core gradually diminishing in intensity towards the outer regions. The galaxy's overall color appears relatively uniform across its structure, suggesting a population of older stars. There is no obvious evidence of spiral arms or prominent dust lanes. The shape is somewhat elongated, with a slight deviation from a perfect circular profile. There are no prominent features of active star formation visible in this image. No signs of strong gravitational disturbance or tidal interactions with nearby galaxies are apparent.
