The galaxy presents a spiral structure, although it appears somewhat face-on, limiting the clear visibility of defined spiral arms. The central bulge exhibits a concentrated luminosity, suggesting a significant stellar population. The disk surrounding the bulge displays a bluer hue, possibly indicative of ongoing star formation. The overall structure appears relatively undisturbed, showing little evidence of major mergers or significant tidal interactions. The galaxy's shape is mostly rounded, leaning slightly towards an in-between ellipticity. Some minor disturbances appear within the spiral arms, and it does not seem to be undergoing any major merging events.
