The galaxy presents as a somewhat diffuse object with a dominant central bulge. The galaxy exhibits an overall elliptical morphology, appearing more rounded than elongated. There is a hint of a disklike structure present in the galaxy, but the bulge is noticeably the dominant feature. The light distribution within the galaxy appears smooth, with little evidence of strong spiral arms or significant dust lanes. The color profile suggests a stellar population with a mix of ages; the bulge appears more yellow/orange, indicating older, redder stars, while the possible faint disk exhibits bluer hues, possibly indicating on going star formation. There is evidence of some kind of galactic interaction or merger based on the overall morphology and shape. The object appears to be at a considerable distance, and is relatively compact.
