The galaxy presents as a relatively smooth, centrally concentrated object. It appears to have an elliptical morphology, with the light distribution diminishing gradually from the core outwards. The core region exhibits a yellowish-white hue, suggestive of an older stellar population dominating the central regions. Moving outwards, the galaxy subtly transitions to a bluer color profile. There is no clear evidence of distinct spiral arms or a prominent disk structure in the image. Overall, the galaxy appears as a fairly undisturbed system, with no major signs of ongoing mergers or significant tidal disturbances, although a very subtle asymmetry could hint at a minor gravitational interaction.
