The galaxy presents as a centrally concentrated object, with a smooth, elliptical morphology exhibiting a dominant yellowish hue in the core, transitioning to a more diffuse outer region. There is no discernible spiral arm structure visible. The galaxy appears to be moderately luminous. There is a slight elongation in shape, suggesting it could be classified between round and cigar shaped. Based on the color, it is likely a relatively evolved galaxy with an older stellar population. There is no obvious evidence of a recent major merger, although minor disturbances cannot be ruled out. Based on the light profile, it is estimated that the galaxy is ~10 kpc across in size. Star formation appears low in the object.
