This galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution. The galaxy's core presents a bright, concentrated luminosity that gradually diminishes outwards. Its overall shape is generally rounded. There are no obvious spiral arms or distinct dust lanes visible, which further supports the classification of this galaxy as an elliptical type. There is some evidence of minor disturbances within the galaxy's structure, though no obvious signs of an ongoing major merger. A faint haze extends well beyond the galaxy's central region. The galaxy exhibits a slightly redder hue, suggestive of a population of older stars and lower rates of star formation.
