The galaxy presents a generally smooth, rounded morphology. A central bulge region is apparent, exhibiting a yellowish hue, indicative of an older stellar population. Fainter, bluer extensions surround the central bulge, suggestive of ongoing, albeit subdued, star formation activity within the galaxy's outer regions. No prominent spiral arm structures or distinct features such as bars or rings are discernible. There is a subtle asymmetry on one side, possibly a minor gravitational disturbance. Overall, the galaxy appears relatively undisturbed and evolved.
