The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable color gradient, with the central region exhibiting a more yellow-orange hue, suggesting a population of older, redder stars. Moving outwards from the core, the color shifts towards a slightly bluer tone, indicating the presence of a younger stellar population, although to a lesser extent. The galaxy does not show any prominent spiral arms or a well-defined disk. The overall shape is neither perfectly round nor particularly elongated, appearing somewhat in between. There is no strong evidence of ongoing major mergers or significant tidal disturbances.
