The galaxy appears to be a relatively compact, disk-shaped system, seen at a near edge-on orientation. A central bulge is visible, appearing bright and yellowish. This is surrounded by a fainter and broader disk, colored with tinges of green, likely indicating areas of star formation. Redder hues are visible on the edge of the central bulge, implying the presence of dust lanes or obscured regions in the inner disk. There appears to be minimal evidence of major disturbances, such as tidal tails or significantly distorted morphology, though there may be some slight unevenness in the outer disk regions, particularly with an asymmetry on the disk. Overall, the galaxy exhibits a relatively undisturbed and well-defined structure.
