The galaxy presents as a centrally concentrated, elliptical-like object, exhibiting a smooth morphology with no obvious spiral arm structures or prominent dust lanes. The light profile appears generally symmetrical, with the brightest region located at the galactic center. The color gradient suggests a relatively old stellar population, showing a yellowish hue indicative of evolved stars. There is little evidence of ongoing active star formation; it appears to be a quiescent galaxy. A slight ellipticity is observed, but the galaxy is primarily rounded in shape. There is no readily apparent evidence of any major tidal disturbances or recent merger activity, although minor asymmetries cannot be ruled out due to the image resolution. Overall, it has characteristics of a mature and relatively undisturbed system.
