The object appears to be a relatively compact galaxy. It exhibits a bright, concentrated central region, possibly indicative of an active galactic nucleus or a dense stellar population. The overall shape is somewhat irregular, deviating from a perfectly elliptical or spiral structure. There seems to be a faint, diffuse halo surrounding the central concentration, though its extent and structure are difficult to discern. There is a hint of disturbance present in its morphology. The colour profile suggests varying stellar populations, with bluer hues possibly indicating younger, hotter stars, and redder hues hinting at older populations. No clear spiral arm structure is observed.
