The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The morphology appears to be elliptical, with an intermediate degree of ellipticity. There is a dominant, luminous core region, surrounded by a less luminous, extended halo. Faint, disturbed features are observed in the surrounding disk. Some light appears to show traces of red, possibly indicating older stellar populations. There is a hint of bluer light in some of the featured structures, which could suggest recent or ongoing star formation. There is no clear evidence of a major merger.
