The galaxy appears to be a relatively luminous, early-type spiral galaxy with a prominent bulge. The bulge exhibits a smooth, yellowish color, indicative of an older stellar population and minimal on-going star formation. There is a noticeable disk component surrounding the bulge, though it is not tightly wound. The disk shows hints of spiral arm structure with bluer hues, suggesting the presence of younger, hotter stars and some ongoing star formation, although at a moderate rate. The overall shape is somewhat elongated, appearing more in between round and cigar shaped, and the galaxy shows evidence of minor disturbances or interactions in its structure but is not currently undergoing a major merger.
