The galaxy appears as a relatively smooth, elliptical object, showing a concentrated central bulge. There's a slight elongation of the galaxy's overall shape. The light distribution suggests a fairly homogenous stellar population, with a gradual decrease in brightness from the core to the outer regions. The overall color profile appears consistent with an older stellar population, lacking prominent features indicative of active star formation, though there is faint blue light detectable. Possible minor disturbances are observed. No distinct spiral arms or significant dust lanes are apparent in this image.
