The galaxy presents as a centrally concentrated, roughly circular form. It exhibits a smooth, diffuse light distribution, suggestive of an elliptical morphology, with no apparent spiral arm structure or distinct disk features visible in this image. The core appears brighter and more compact than the surrounding region, with a gradual decline in intensity moving outwards. The overall color appears to be consistent with an older stellar population, with hints of redder hues in the central region and slightly bluer tones in the extended halo. There are no visible signs of ongoing major mergers or significant tidal disturbances.
