The galaxy presents a fuzzy, unresolved appearance. Its morphology suggests an elliptical or lenticular type, exhibiting a generally smooth light distribution, though subtle variations hint at possible underlying structure. There may be some early signs of a minor merger or tidal disturbance. The primary body of the galaxy is largely spheroid with a slightly off-centered, more luminous core. The lack of distinct spiral arms or significant dust lanes suggests an older stellar population, with moderate ongoing star formation. The overall color is yellowish-white, which is consistent with a substantial population of evolved stars. There is some possible evidence of a faint tidal tail or plume extending from the main galactic body, indicating gravitational interaction with a smaller companion or previous merger event.
