This galaxy exhibits a somewhat elongated shape, with a noticeably concentrated central bulge that appears yellowish-white in color, potentially indicating an older stellar population. Diffuse blue light extends from the central region, suggesting the presence of some ongoing star formation within its structure. The galaxy shows a mild disturbance in its morphology, not fitting perfectly into a simple elliptical or spiral classification. It leans towards a smoother structure, with only faint hints of spiral arm features. The overall color suggests a mix of stellar populations, with the bulge being dominated by older, redder stars and the outer regions showing younger, bluer stars.
