The galaxy presents a concentrated central region. There is a smooth, though not perfectly spherical, distribution of light suggesting it is likely an elliptical galaxy. A slight asymmetry is present and there appears to be a region that is less centralized and brighter than the overall profile of the galaxy, which could be an area of ongoing star formation, although the general red hue of the object suggests an older stellar population overall. The galaxy does not appear to be undergoing any major merger events, although there may be some minor disturbances in the light distribution. The galaxy has an estimated effective radius of approximately 5 kpc, indicating that this is not a small, dwarf galaxy. The relatively bright absolute magnitude suggests that this galaxy is luminous, and its mass estimate is around 10^10.5 solar masses.
