The galaxy presents as a centrally concentrated object, with a smooth overall appearance. The majority of light appears to be concentrated in a bright, unresolved core or bulge region. Surrounding this central region is a more diffuse, fainter halo of light that extends outwards. While somewhat circular in overall form, a slight elongation is noticeable along one axis, indicating that it may not be perfectly spherical. There is no obvious spiral structure. The color gradient suggests a relatively older stellar population. Although subtle, there are indications of minor disturbances in its form which could be a merging event. Star formation activity is relatively low. 