The galaxy presents as a flattened, disk-like structure with a pronounced central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population and potentially lower star formation activity in that region. Moving outwards from the bulge, the disk shows a bluer coloration, hinting at the presence of younger, hotter stars indicative of ongoing star formation. While the overall structure appears relatively smooth, there are subtle indications of spiral arm structures within the disk, though these are not sharply defined. The galaxy's elongated shape suggests an inclined viewing angle relative to our line of sight. There is some indication of tidal disturbance, in a faint, slight extension of galactic material to the right, suggesting past or ongoing gravitational interactions with another galaxy.
