The galaxy appears as a moderately compact structure, elongated in shape. It displays a relatively smooth, diffuse light distribution, with a slight variation in color across its body. A subtle color gradient is observed, with a hint of bluer tones concentrated in the central regions, transitioning toward redder hues in the outer parts. This could indicate some ongoing or recent star formation activity near the core. There is no clear evidence of spiral arm structure or a prominent central bulge, suggesting it could be a lenticular or elliptical galaxy viewed at an oblique angle. There are no obvious signs of recent major mergers or tidal disturbances.
