The galaxy presents an elliptical morphology, appearing as a generally smooth, centrally concentrated object. Its overall color profile suggests an older stellar population, with a dominant yellowish hue concentrated in the central bulge. A subtle flattening is visible, indicating a degree of rotation. Faint, diffuse extensions are noted, implying possible tidal interactions. The presence of sparse bluer regions suggests ongoing but limited star formation. No obvious spiral arms or bar structures are detected.
