The galaxy appears as a relatively small, diffuse object with a smooth, elliptical morphology.  There's a centrally concentrated brightness that gradually fades towards the outer regions. No distinct spiral arms or prominent dust lanes are discernible.  The light distribution suggests an older stellar population with minimal ongoing star formation activity.  The overall structure is quite regular, showing no signs of major tidal disturbances or recent merger events, though a very faint asymmetry could indicate minor interaction. The color appears generally red, consistent with a population of older, redder stars.
