The galaxy presents a relatively smooth and concentrated morphology. The central region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. There's a gradual fading of color intensity and light as we move towards the outer edges, which appear somewhat irregular but lack defined spiral arm structures. The overall shape suggests a possible elliptical or lenticular classification, though there might be a faint, diffuse disk component that is not clearly resolved. There is no obvious active galactic nucleus or other high-energy phenomena visible. The smooth appearance suggests this galaxy is well-relaxed. No signs of tidal tails or ongoing interactions are evident in this image, however there appears to be some minor disturbance.
