The galaxy presents as a centrally concentrated object with a largely smooth morphology. There is evidence of a slight elongation, although the overall form appears close to circular. The primary color is a relatively consistent yellow-white, with a slightly bluer halo surrounding a more centrally localized concentration. Within the central region there is some suggestion of internal structure, potentially related to dust or gas clouds, although the resolution is insufficient to determine its precise nature. There are no prominent spiral arms or a distinct central bar, indicating a possible early-type or lenticular classification. There appears to be little to no major interaction or merging activity with nearby galaxies, or evidence of substantial disturbances.
