The galaxy presents as a single, relatively smooth object with a generally elliptical morphology. The color profile appears more concentrated towards the center, displaying a yellowish hue that suggests an older stellar population. The outer regions of the galaxy appear fainter and exhibit a slightly bluer tint, potentially indicating the presence of some younger stars or residual star formation. There is no obvious spiral structure, bar, or significant dust lane visible, suggesting a classification towards the elliptical or lenticular end of the Hubble sequence. The object exhibits a high degree of central concentration with a relatively even surface brightness distribution, implying a well-mixed stellar population and advanced stage of morphological evolution. There is no clear evidence of tidal disturbances or ongoing mergers in this image.
