The galaxy appears to be a relatively smooth, elliptical structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population. A bluer halo surrounds the bulge, indicating the presence of younger, hotter stars potentially within a disk structure. The overall shape is elongated, appearing more 'in between' round and cigar shaped. There's no obvious presence of spiral arms or dust lanes. No significant signs of major interaction or merging activity are apparent, although a minor disturbance might be possible given the slight asymmetry in the outer regions.
