The galaxy presents as a centrally concentrated, relatively smooth object with a slight elongation. A dominant central bulge is visible, exhibiting a yellowish hue. This coloration suggests an older stellar population dominating the core. The galaxy displays a smooth falloff in intensity from the center outwards, indicative of a lack of prominent spiral arm structures or significant dust lanes. There is faint bluer light that is slightly extended around the yellow core. The overall morphology leans towards elliptical or S0-type, though deeper observations would be necessary to confirm. The lack of strong blue emission suggests a low star formation rate. There does not appear to be any signs of ongoing mergers or major tidal disturbances.
