The galaxy exhibits a generally elliptical morphology. Its light profile appears relatively smooth and centrally concentrated. There is a slight elongation, but the aspect ratio does not suggest a highly flattened structure. The core region displays a yellowish hue, potentially indicating a population of older stars. Fainter, bluer light is observed in the outer regions of the galaxy, this may point to the presence of ongoing or recent star formation. There's a hint of disturbed features or tidal tails, but the disturbance appears minor.
