The galaxy presents a largely smooth morphology, exhibiting a central bulge that is brighter and more concentrated than the surrounding regions. There is a noticeable color gradient from the core outwards, with the central region appearing yellower, suggestive of an older stellar population. The outer regions show hints of bluer hues, possibly indicating some level of ongoing, albeit relatively subdued, star formation. The galaxy's overall shape is elliptical, deviating slightly from perfect roundness. There is no apparent strong disk structure or evidence of major ongoing mergers or significant tidal disturbances. Subtle irregularities in the galaxy's outer envelope may hint at past interactions or minor disturbances, but these features are not prominent. The overall impression is of a relatively evolved system, transitioning towards a red and dead state with a gradually declining star formation rate.
