The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. The overall color appears to be a yellowish-orange, which may indicate an older stellar population with fewer young, massive stars. There is little evidence of distinct spiral arms or significant dust lanes, suggesting a lack of ongoing, widespread star formation. The galaxy exhibits a high degree of central concentration, with light intensity decreasing gradually from the core to the outer regions. It appears largely undisturbed, showing no prominent signs of tidal features or morphological disturbances indicative of recent major merger activity, though there may be some minor disturbances. The galaxy appears to have a high degree of symmetry, tending towards round.
