The galaxy presents as a relatively smooth, elliptical structure. Its light profile is centrally concentrated, exhibiting a gradual decrease in luminosity from the core outwards. The core itself appears to be slightly brighter and more yellow-white in color, possibly indicating an older stellar population. The outer regions of the galaxy show a somewhat fainter, diffuse halo, gently bluer in color. There is minimal evidence of distinct spiral arms or significant dust lanes. The galaxy appears slightly elongated, leaning more towards an "in-between" rounded shape. There is no obvious signs of on-going major merger activity or significant tidal disturbances. Overall, the galaxy appears as a quiescent system, dominated by an older stellar population, with limited ongoing star formation.
