The galaxy presents as a concentrated, largely homogenous light source. The morphology appears elliptical, with a smooth, diffuse profile, and is nearly circular in appearance. The galaxy core exhibits a significantly brighter, yellowish hue, which gradually fades outward, transitioning to a more bluish tint in the outer regions. There are no prominent dust lanes, spiral arms, or other distinct features readily apparent. The galaxy does not seem to be undergoing a major merger or experiencing any significant tidal distortions based on its apparent form. There may be subtle, minor disturbances present. Star formation appears to be occurring, but not at a high rate. Overall, the galaxy appears to be relatively quiescent and well-ordered.
