The galaxy presents as a relatively smooth, elongated structure. Its morphology appears elliptical, deviating significantly from a spiral or irregular form. The light distribution is centrally concentrated, with a gradual decrease in brightness moving outwards. The galaxy exhibits a subtle color gradient, appearing slightly redder in its core and becoming marginally bluer towards its outer regions. No distinct spiral arms or dust lanes are discernible in the image. There are no apparent signs of ongoing major mergers or significant tidal distortions. Any minor disturbances are subtle, and the galaxy appears relatively isolated. The overall impression is that of a mature, relatively quiescent system.
