The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a centrally concentrated light profile. Its shape is generally round, showing minimal deviation from circular symmetry. The galaxy presents a yellow-orange hue, suggesting an older stellar population with fewer young, massive stars contributing to the overall light output. There is no apparent spiral structure, disk component, or evidence of ongoing major mergers or significant tidal disturbances. Subtle irregularities in the outer regions could suggest past minor interactions, but the dominant morphology indicates a relaxed, relatively evolved system. The galaxy is compact and of intermediate size. Overall, this galaxy appears to be an elliptical galaxy that is old and has had no recent major disturbances.
