The galaxy presents as a somewhat amorphous structure with a diffuse central region and less defined spiral arms. There is a subtle color gradient, with the core appearing slightly redder and the outer regions showing hints of bluer light, potentially indicating ongoing star formation. The galaxy is moderately bright and has a small, angular size, suggesting it is relatively distant. There is no obvious bar structure or strong central bulge. The overall light distribution suggests an intermediate type between a pure elliptical and a well-defined spiral, possibly an early-type spiral or a lenticular galaxy undergoing some star formation. No distinct dust lanes are readily apparent, and there is a subtle feature to the lower side of the galaxy that might indicate a minor interaction or disturbance, however, this is difficult to tell from the image itself.
