The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The light distribution suggests a roughly elliptical shape, although not perfectly round. The core region appears significantly brighter and more intensely luminous than the outer regions, indicating a possible concentration of older stellar populations in the central bulge. There's a hint of asymmetry in the light distribution, with a faint, diffuse extension or possible minor disturbance visible on one side. The overall color appears to be a yellowish hue, possibly indicating a lack of significant ongoing star formation. There is little evidence of prominent spiral arms or a well-defined disk structure, though one cannot be ruled out.
