The galaxy presents as a relatively smooth and concentrated structure. There is little evidence of distinct spiral arms or a well-defined disk. The overall morphology appears to be elliptical. The galaxy exhibits a gradual color gradient, transitioning from a brighter, yellowish core to a fainter, slightly redder outer halo. This color distribution could be indicative of an older stellar population dominating the central region. The symmetrical shape suggests it is unlikely to be undergoing a major merging event, although there is some asymmetry to the halo.