The galaxy presents a generally smooth, elliptical morphology. It appears elongated, exhibiting a cigar-like shape. The galaxy lacks any readily discernible spiral arm structures or strong irregularities, suggesting a relatively featureless disk if present. The central region is noticeably brighter and more concentrated than the outer regions, indicating a distinct galactic nucleus. Based on the color profile and lack of visible dust lanes, the galaxy likely has a modest star formation rate. There is no apparent interaction or merging activity ongoing with neighboring galaxies.
