The galaxy presents as a relatively smooth, concentrated object. Its overall form is generally elliptical, appearing mostly round with a very subtle elongation. The color profile is consistent with an older stellar population, exhibiting a yellowish-white hue in its core, suggesting evolved stars dominate the light output. There is some indication of bluer regions extending from one side of the central bulge, potentially indicating areas of more recent star formation. There may be minor disturbances affecting the galaxy's morphology. The galaxy is relatively isolated in the observed field, not exhibiting any obvious signs of on-going merger activity, though a minor disturbance may be present.
