The galaxy presents a largely smooth morphology, indicative of an elliptical or lenticular type. It appears moderately concentrated, with a bright central bulge that gradually fades into a less luminous halo. The color profile suggests a dominant population of older stars, evidenced by the yellowish-red hue of the core. There's a hint of bluer light in a small area to the left of the galaxy, implying a possible region of younger star formation. The overall structure doesn't show any prominent spiral arms or significant dust lanes. There are some minor disturbances possibly indicating some sort of interactions with other galaxies. The galaxy's shape is roughly elliptical, but slightly distorted.
