The observed galaxy appears to be a disk galaxy, though it is not face-on, presenting at a slight angle relative to our line of sight. There is a notable bulge, characterized by a smooth, concentrated luminosity gradient towards the central region. The disk is visible, with some suggestion of spiral structure, though the resolution is limited. There is a hint of asymmetry in the outer regions of the disk, possibly indicating a minor interaction or disturbance. The galaxy exhibits a broad color gradient, with the central bulge appearing more yellow/red, indicative of an older stellar population. The disk shows bluer regions, particularly within the spiral arm segments, suggesting ongoing star formation. There is also a hint of dust obscuration present. Overall, the galaxy presents a generally smooth appearance, with some indication of underlying complexity in its structure and stellar populations.
