The galaxy exhibits a pronounced disk structure, viewed at a significant inclination. This is evidenced by the flattened elliptical shape and the distinct layering of light intensity. The central region appears brighter and more concentrated, suggesting a substantial bulge component. Faint spiral arm structures are visible, though not sharply defined. Dust lanes appear to be present, but only subtly, and not with great clarity. The overall color profile indicates a galaxy populated with a mix of stellar populations. The bulge appears more yellow/red, suggesting older stars, while the outer disk regions show bluer hues, possibly indicating regions of active star formation. The galaxy appears relatively isolated with no obvious signs of ongoing mergers or significant tidal interactions with nearby galaxies.
