The galaxy presents as a moderately inclined, disk-shaped system. The central region appears brighter and more concentrated, suggesting a prominent bulge. The color profile indicates a relatively old stellar population, with a yellowish-white hue dominating the core and inner disk, trending slightly bluer towards the outer edges. This gradient could indicate ongoing, though perhaps limited, star formation in the periphery. There is little evidence of tightly wound spiral arm structure; the galaxy appears mostly smooth, possibly a lenticular (S0) type or a tightly wound spiral galaxy viewed at a distance where such structures become difficult to resolve. There is no obvious dust lane bisecting the disk. The overall shape is elongated, with a significant difference between the major and minor axes, indicating a non-circular morphology. There are no clear signs of recent major merger events or strong tidal interactions affecting the visible structure.
