The galaxy presents an elongated, disk-like morphology, suggesting it is likely a spiral or lenticular galaxy viewed at an oblique angle. A bright central bulge is visible, exhibiting a yellowish hue that may indicate an older stellar population. The galactic disk displays a complex structure with hints of spiral arm features, though the resolution is not sufficient to resolve individual star-forming regions or dust lanes. The color gradient across the disk suggests a radial variation in stellar populations, with bluer colors towards the outer regions, potentially indicating ongoing star formation. The galaxy lacks any obvious signs of recent major mergers or strong tidal interactions, although subtle asymmetries in the disk structure might suggest minor disturbances. The overall impression is of a relatively mature galaxy undergoing normal evolutionary processes.
