The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. Its shape appears nearly spheroidal, exhibiting minimal elongation or disk-like features. The galaxy exhibits a yellowish-white color, suggesting an older stellar population with a relatively low rate of ongoing star formation. There is no evidence of prominent spiral arms, bars, or other distinct features typically associated with late-type galaxies. No tidal features or significant morphological disturbances are detected, indicating that it is most likely not undergoing a major merger. A possible minor interaction cannot be ruled out.
