The galaxy presents as a centrally concentrated object, with a relatively smooth overall appearance. The core region exhibits a bright, somewhat yellowish hue, suggesting a population of older stars. Moving outwards from the core, a subtle transition towards a greenish-blue color is observed, possibly indicating some level of ongoing star formation in the outer regions. There are hints of faint reddish patches along the periphery, potentially signifying areas with dust or older stellar populations. The galaxy appears to be generally elliptical or spheroidal in shape, with no obvious signs of a disk structure or spiral arms. There is no strong evidence of any major disturbances or mergers; the system appears relatively relaxed and undisturbed.
