The galaxy presents a moderately inclined disk structure. The central bulge appears luminous and somewhat spheroidal, exhibiting a yellowish-white hue, possibly indicative of an older stellar population. The disk component, although partially obscured by the inclination, appears to extend outwards from the bulge. There is a subtle color gradient visible from the central bulge towards the outer regions of the disk. Some faint blueish clumps are observed in the disk region. These may be areas of ongoing star formation. The overall morphology seems relatively undisturbed, with no obvious signs of major mergers or tidal interactions, although a minor disturbance cannot be ruled out. The galaxy has a smooth appearance, indicating the majority of light is from older stars.
