The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of central symmetry and no obvious spiral arm structure, bars, or pronounced disk component. There is some indication of a faint, diffuse halo extending beyond the brighter central region. The color gradient suggests a population dominated by older stars, with the central regions exhibiting a yellower hue and the outer regions appearing slightly bluer. Evidence for recent or ongoing star formation is not prominent. The overall structure suggests that any merger activity in its recent past would not have been major, but some minor disturbances are possible. It exhibits a somewhat round shape overall, with no significant elongation.
