The galaxy presents as a somewhat elliptical, luminous object, approximately 7 kpc in radius based on estimations from the provided data. Its central region exhibits a concentrated, bright yellowish glow, potentially indicating a population of older stars. The outer regions display a more diffuse, fainter greenish hue, with a slight color gradient moving from the center outwards. There are no apparent spiral arm structures or significant dust lane features visible within the galaxy's morphology, giving it a relatively smooth appearance. Slight distortions or irregularities can be seen in the outer regions, though there is no evidence of an ongoing merger or significant disturbance of any kind. This suggests a system that is relatively relaxed and stable.
