The galaxy presents a predominantly smooth and concentrated appearance. It exhibits a centrally bright bulge that dominates the overall light profile. The bulge appears nearly spherical. The disk component is either faint or highly inclined, contributing a smaller fraction of the total light. The galaxy displays a yellowish hue centrally, suggesting a population of older stars within the bulge. There is a very slight suggestion of bluer light peripherally, hinting at some ongoing star formation, but it is not prominent. There is no obvious evidence of strong spiral arms or a bar structure. There is some minor visual disturbance as well. No other companions or merger events are immediately apparent.