The galaxy presents as a relatively compact object with a centrally concentrated luminosity. The morphology appears to be primarily smooth, with a dominant spheroidal component, suggesting a possible elliptical or lenticular classification. There appears to be some indication of a disk component to the structure. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, potentially indicating an older stellar population, while the outer regions show hints of bluer hues, suggesting the presence of younger stars or ongoing star formation. Faint asymmetric features or tidal tails are also possibly present, indicating interactions or recent merging events, however, the signal is weak and could be background or noise. The object appears to be in a relatively quiescent state of star formation.
