The galaxy presents as a somewhat centrally concentrated, luminous object, exhibiting a generally smooth morphology. The central region appears as a bright, yellowish core, possibly indicative of an older stellar population. Extending outward from the core, a more diffuse, bluish halo is observed, suggesting the presence of younger, hotter stars and possibly ongoing star formation. There is some subtle asymmetry in the outer regions which may be suggestive of a minor gravitational interaction or internal disturbances. The overall shape is elliptical, but appears to be transitioning to a disk shape. Although appearing mostly smooth, the galaxy may be exhibiting disk features. The estimated size is approximately 6 kpc.
