The galaxy presents as an elliptical-like structure, exhibiting a generally smooth morphology with a concentrated central bulge. Its color profile suggests a population of older stars, as indicated by the redder hues dominating its composition, with hints of yellow closer to the center. The galaxy does not exhibit any prominent spiral arms or distinct dust lanes. There appears to be a nearby object but it is unclear if the two are interacting. The main body displays a relatively even light distribution with the highest concentration being the central bulge. There appears to be minimal evidence of active star formation.
