The galaxy presents as a relatively smooth, centrally concentrated object. It appears to have a roughly elliptical morphology, with no immediately discernible spiral arm structures or a distinct bar. There might be a slight extension to one side, suggesting a minor tidal interaction or disturbance. 

The color profile is somewhat redder towards the center, indicating a potentially older stellar population concentrated in the bulge. There is a hint of bluer light in the outer regions of the galaxy, which might suggest ongoing, albeit low-level, star formation. Overall, the galaxy's smooth appearance and redder color profile suggests a potentially evolved system with a significant fraction of older stars.
