The galaxy presents as a somewhat elliptical, disk-like structure. The central region exhibits a concentrated, bright, orange-yellow hue, suggestive of an older stellar population. Surrounding this core is a less concentrated region, showing hints of greenish-blue light which could suggest areas of more recent star formation. The galaxy appears relatively smooth in overall texture, with only minor indications of disturbances or mergers. Its shape deviates noticeably from perfectly circular, elongated and more cigar-shaped. The galaxy exhibits an estimated mass of around 10^10 solar masses. The star formation rate implies that the galaxy is undergoing an active, ongoing star formation process.
