The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a centrally concentrated bulge. There's little to no discernible spiral arm structure. The color profile indicates a dominant population of older stars, with the central region exhibiting a yellowish hue, suggestive of evolved stellar populations. The outer regions of the galaxy become gradually fainter, blending into the background sky. There is no evidence of any major ongoing merger activity or significant tidal disturbances. There is very little, if any, evidence of active star formation. The overall appearance suggests a fairly quiescent galaxy, likely with limited gas content. The angular size implies a moderately large physical extent for a galaxy at its distance.
