The galaxy presents a generally smooth, rounded morphology. Its light is concentrated towards the center with a bright, distinct core. The color profile suggests a population of older stars, presenting as a slightly reddish-yellow hue overall, although there is a slight hint of bluer light in the surrounding halo. There is no obvious spiral structure or prominent disk. There is no clear evidence of ongoing major mergers or tidal disturbances in this image. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity.
