The galaxy presents as an elongated, disk-like structure viewed nearly edge-on. The central bulge region appears bright and concentrated with a yellowish hue, possibly indicating an older stellar population. A flattened disk extends outwards from the bulge, exhibiting a fainter and bluer coloration, suggestive of ongoing star formation. There is some indication of dust lanes, although they are subtle, implying a relatively smooth dust distribution within the disk. Overall, the galaxy seems to be relatively undisturbed with no obvious signs of a major merger or tidal interactions.
