The galaxy presents as a relatively bright, extended object with a noticeable bulge. The bulge appears yellowish-white, suggesting an older stellar population. A faint disk component can be observed extending from the bulge, indicating the presence of a flattened structure. Within the disk, hints of spiral arm structures or dust lanes can be inferred. The overall structure leans towards a spiral or lenticular morphology. The color of the outer disk appears slightly bluer compared to the bulge, indicative of ongoing star formation. There is a possible interacting galaxy close by. There is no significant evidence of a recent major merger event. The galaxy seems to be in a relatively quiescent state of star formation, with a moderate mass.
