The galaxy presents as a centrally concentrated elliptical type. It exhibits a smooth, largely featureless morphology, with a high degree of central concentration gradually decreasing in luminosity outwards towards its indistinct edges. The galaxy's shape appears mostly round. The color profile is dominated by yellow and red hues, suggesting an older stellar population with diminished star formation activity. There are no visible signs of spiral arms, bar structures, or significant dust lanes. There is also no readily apparent sign of any ongoing major merger activity or tidal disturbances. The galaxy seems to be relatively isolated in the field of view and appears relatively undisturbed.
