The galaxy presents a generally smooth morphology, with a concentrated central region of high luminosity. Its shape appears largely elliptical, deviating minimally from a circular profile. There is no evident spiral arm structure or significant dust lane obscuration, suggesting a relative lack of ongoing star formation. The color profile indicates a higher concentration of older stellar populations. No distinct tidal features or signs of recent merger activity are observed. The overall appearance suggests a classification toward the early-type end of the Hubble sequence, potentially an elliptical or lenticular galaxy at intermediate redshift.
