The galaxy appears to be an elliptical or lenticular type, characterized by a smooth, featureless morphology. The central bulge exhibits a concentrated, bright yellowish hue, suggesting a population of older stars. Moving outwards from the core, the color transitions towards a slightly bluer tint, although overall, the galaxy retains a relatively uniform color distribution. There's no obvious evidence of spiral arms, bar structures, or significant dust lanes. The isophotes appear mostly regular, indicating a relaxed system without signs of recent major mergers or strong tidal interactions. The galaxy's shape appears roughly circular. Overall, the observed characteristics suggest a galaxy dominated by an older stellar population, possibly with ongoing but relatively low levels of star formation.
