The galaxy presents as a relatively smooth, single structure with a concentrated central bulge. The light distribution suggests an elliptical morphology, although a slight disky component cannot be entirely ruled out. The color gradient shows a central, yellowish-orange hue, indicative of an older stellar population, surrounded by a bluer halo, suggesting the presence of some younger stars and ongoing, albeit potentially low, star formation. There is no apparent sign of any ongoing major merger events or strong tidal disturbances. There might be a slight asymmetry in the outer regions, possibly suggestive of a minor interaction or subtle internal feature.
