The galaxy presents as an elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. It is largely featureless with a centrally concentrated bulge. The color profile suggests a population of older stars, indicated by the reddish hue of the central region, potentially mixed with intermediate age stars appearing greenish/yellow. The galaxy does not appear to be undergoing any major merger activity or significant tidal disturbances based on visual inspection. The round shape is indicative of a relatively relaxed system that has not been significantly perturbed recently.
