The galaxy presents as a single, centrally concentrated object, exhibiting a smooth, elliptical morphology. Its color profile suggests an older stellar population, with a yellowish-red hue indicating a relatively quiescent galaxy. There is no apparent spiral arm structure, bar, or dust lane visible at this resolution. The overall form is quite regular, showing no signs of major tidal disturbance or ongoing merger activity, though there is a possible minor disturbance. The galaxy's round appearance indicates it likely lacks a significant disk component. The size appears relatively compact.
