The galaxy presents as a slightly elliptical, centrally concentrated structure. The central bulge appears a more yellowish hue, suggestive of an older stellar population. The outer regions show a hint of bluer colors, especially on the edges, possibly indicating areas of recent or ongoing star formation. The overall form is largely smooth, with no obvious spiral arm structure or significant dust lanes visible in this image. There appears to be a slight asymmetry and some distortion in the galaxy’s halo. The galaxy's overall morphology appears to be that of a relatively undisturbed system that may be potentially undergoing a minor merger. The galaxy has very low star formation activity. 
