The galaxy presents as an elongated, somewhat disturbed system. It appears to be a disk galaxy viewed at a moderate inclination. The color profile suggests a significant population of older stars, imparting a yellowish hue to the galaxy. The disk's morphology indicates a complex structure, possibly exhibiting subtle tidal features or internal disturbances, suggesting past or ongoing interactions. Star formation appears subdued throughout, with no prominent HII regions or strong concentrations of young, blue stars visible. The overall impression is of a galaxy that has undergone significant dynamical evolution.
