This galaxy appears to be an elliptical galaxy, characterized by a smooth, round, and centrally concentrated luminosity profile. It presents with a dominant yellow-orange hue, suggesting an older stellar population and minimal ongoing star formation. There is a high degree of central concentration, with the light intensity gradually decreasing outwards. Close inspection reveals some subtle color variations. There's a hint of bluer regions, suggesting a possible area of star formation. A small, redder region is also present, possibly indicative of dust or a region of older stars. There's no clear evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, exhibiting no signs of major mergers or significant tidal interactions.
