The galaxy presents as a resolved object with an elliptical morphology. It exhibits a smooth appearance, lacking prominent spiral arms or a well-defined disk structure. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region occupying a significant portion of the galaxy's area. There is some color variation, with a dominant yellowish-orange hue in the central region transitioning to a slightly bluer tint towards the periphery on one side. This may indicate the presence of older stellar populations in the core and potentially some more recent star formation activity in the outer regions. There is also some indication of a possible interaction or minor disturbance on one side, based on the overall morphology. The galaxy's estimated size suggests it is a fairly large system. Overall, this galaxy appears to be a massive elliptical galaxy at a considerable distance.
