The galaxy presents a generally smooth morphology. The light distribution suggests an elliptical shape or possibly a lenticular galaxy seen face-on. The central region exhibits a concentrated bright core. Moving outwards, the light gradually diminishes, with no distinct spiral arms or prominent disk-like structures discernible.

The color profile indicates an older stellar population, evidenced by the dominant reddish-yellow hue. Star formation appears to be suppressed throughout the galaxy. There is no indication of active merging events or major disturbances to the galaxy's overall structure. Small deviations are potentially present in its structure which could indicate a past minor merging. The overall appearance indicates it is a massive galaxy.
