The galaxy presents as a moderately luminous, elliptical or lenticular system at a redshift of approximately 0.15. Its overall form appears relatively smooth with no prominent spiral arms or distinct dust lanes visible, although the colors are somewhat heterogenous, suggesting some degree of internal structure. The galaxy appears to have a central concentration of light, with the intensity gradually diminishing towards the edges. It appears mostly spherical, and does not show evidence of active merging or tidal disruptions, though some minor asymmetry can be detected, implying that it might be interacting with another galaxy. It exhibits color gradients, with a redder core possibly indicating an older stellar population or increased dust obscuration. Fainter extended emission surrounds the main body. Given its characteristics, the galaxy likely has a mass range that is within a normal range for galaxies at this redshift. Finally, the galaxy appears to have a fairly low star-formation rate.
