The galaxy appears as a single, relatively smooth object with a concentrated central region. The light distribution suggests an elliptical morphology, possibly an early-type galaxy. The color is yellowish-white, indicating a stellar population dominated by older stars. There is no visible spiral structure or dust lanes. The galaxy exhibits a high degree of roundness with no apparent disturbances, indicating it is likely not undergoing any major merger events. The absence of significant blue light suggests limited ongoing star formation. The estimated size indicates that it is a relatively large galaxy, but with no distinct features besides the central bulge.
