The object presents as a relatively smooth, centrally concentrated galaxy. It exhibits a predominantly elliptical morphology with a high degree of radial symmetry. The galaxy's color profile suggests a bulge dominated system, showing a yellowish-orange hue indicating an older stellar population. There is no visible evidence of spiral arms or a distinct disk structure within the limits of image resolution. Slight asymmetry in the outer regions may suggest minor gravitational interactions, but there is no clear sign of an ongoing merger event, tidal tails, or other major disturbances. Overall, this appears to be a fairly evolved galaxy with a relatively low star formation rate.
