The galaxy presents a centrally concentrated morphology. The core exhibits a yellowish hue, indicative of an older stellar population. Extending outwards from the central region is a fainter, bluish disk structure. This disk appears relatively smooth with no well-defined spiral arms. The overall shape of the galaxy is elliptical but close to round. There are hints of some minor disturbances in the outer regions, potentially suggesting past minor merger events or tidal interactions, but the overall impression is one of relative dynamical quiescence.
