The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with a distinct yellow-white hue in the core, suggesting an older stellar population dominating the nuclear region. A gradual color gradient is observed moving outward from the core, with the outer regions showing slightly bluer colors. The overall shape is elliptical, but appears to be more of an in between roundedness or oval, as opposed to perfectly circular or cigar shaped. There is no clear evidence of spiral arm structure or significant dust lanes present. Overall, the galaxy's morphology suggests it is likely a quiescent system, possibly having undergone significant star formation in the past, but with a lower rate of ongoing star formation. There are no readily apparent signs of strong tidal interactions or major merging events in its recent history, although it cannot be ruled out that it may have undergone a minor disturbance.
