The galaxy appears to be a relatively smooth, elongated structure, suggestive of an elliptical galaxy or a spiral galaxy viewed edge-on. The central region exhibits a concentrated, bright yellowish hue, possibly indicating an older stellar population and minimal current star formation activity. The outer regions display a fainter, more diffuse light, with a slight bluish tint discernible, suggesting a component of younger, hotter stars, though this is minimal compared to the core. There is no clear evidence of spiral arms or significant dust lanes from this angle. The galaxy does not appear to be undergoing any major merging activity or significant tidal disruption.
