The galaxy presents as a disk-dominated system, observed at a high inclination angle relative to our line of sight. The morphology suggests a classification between an elliptical and spiral galaxy, potentially an early-type spiral. The central bulge exhibits a concentrated, smooth distribution of light. The light suggests an older stellar population. Faint and indistinct features that could be spiral arm segments hint at ongoing, though potentially low, levels of star formation within the disk. The overall color profile is red, suggesting a high fraction of older stars and/or significant dust extinction.
