The galaxy presents as a somewhat elliptical, smooth structure with a diffuse profile. The primary color appears to be a pale blue, suggesting the presence of a population of relatively young, hot stars. There is a slight elongation observed, though the overall shape leans toward round. No distinct spiral arms or prominent dust lanes are discernible at this resolution. The galaxy exhibits a soft, fading edge, which implies that it lacks a sharp boundary and possesses a stellar halo or extended envelope. Possible tidal features are not visible. The galaxy does not appear to be currently undergoing any major merger activity.
