This galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular type. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the light gradually fades into a more diffuse, reddish-orange halo, possibly indicating a population of cooler, redder stars in the outer regions. There's a hint of a subtle disk-like structure extending horizontally, though the galaxy's overall form is more spheroidal than flattened. There does not appear to be any spiral arm structure visible, and there's no significant evidence of dust lanes or prominent star-forming regions within the galaxy itself. A minor asymmetry is observed on the lower left quadrant of the galactic halo, perhaps indicative of a tidal interaction, past or present, but no major merger events appear obvious. Overall, the galaxy appears as an evolved system with relatively low ongoing star formation.
