The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated light distribution. Its shape is elongated, with a roughly cigar-shaped appearance. The light profile decreases gradually from a bright core, suggesting an older stellar population. There is a faint blue halo surrounding the main body of the galaxy. No distinct spiral arm structures or prominent dust lanes are discernible in this image. The overall morphology indicates a system that is likely experiencing relatively low star formation activity. The lack of significant morphological disturbances suggests that the galaxy is not currently undergoing a major merger event.
