The galaxy presents as a single, somewhat amorphous entity with a dominant, spheroidal morphology. The light profile appears smooth and concentrated, with a high degree of central light concentration. The overall color is yellowish-orange. There is some subtle indication of tidal structures that would imply a possible ongoing interaction or a recent merger event, which is supported by the irregular shape. There also appears to be a secondary nucleus or an area of increased light.

The galaxy's estimated size is approximately 10.6 kpc. It is emitting strongly in the redder wavelengths, and less so in the blue, suggesting a relatively older stellar population. The calculated values for Star Formation Rate (SFR) and Specific Star Formation Rate (sSFR) indicate that this galaxy has minimal star formation. Finally, the galaxy has an estimated mass of around 10^11.5 Solar Masses.
