The galaxy presents as a largely featureless, elliptical object. It exhibits a smooth, centrally concentrated light profile with a gradual decline in brightness outward from the core. The galaxy appears nearly circular, with only a slight elongation, and does not show any obvious spiral arm structures or prominent dust lanes. Its color is generally red, indicating a population of older stars with limited current star formation. There is no evident sign of ongoing merger activity or significant tidal disturbances, although the possibility of subtle, unresolved interactions cannot be entirely ruled out based on this image alone. The galaxy's overall morphology suggests it is a relatively evolved system, consistent with a lack of substantial star formation.
