The galaxy exhibits a roughly elliptical morphology, with a noticeable elongation along its major axis. The luminosity profile appears concentrated towards the center, decreasing gradually outwards. The color gradient suggests a central bulge with older stellar populations, indicated by the yellower hue, transitioning to bluer regions toward the edges. There appears to be some minor disturbance or asymmetry in the overall shape, possibly indicating a past or ongoing interaction. A slight tidal tail or extended feature is suspected but not clearly defined. The central region is relatively smooth in appearance, while the outer regions display more complex structures, suggesting the presence of spiral arms or irregular features.
