The galaxy presents a generally smooth, elliptical morphology. Its light distribution is centrally concentrated, exhibiting a relatively uniform radial decrease in intensity without prominent spiral arms or a distinct bar structure. There may be some broad, faint disks but they are not distinct. The core appears to be redder in color than the outer regions, suggesting the presence of an older stellar population in the center. The outer regions show bluer colors. There is some evidence of possible minor disturbances, but the galaxy maintains a relatively relaxed appearance without strong signs of on-going major mergers or tidal interactions. The galaxy is moderately sized.
