The object appears as a single, relatively smooth, and luminous galaxy, exhibiting a generally elliptical morphology. The central bulge is prominent and dominates the overall luminosity, displaying a strong yellow/orange hue, suggesting an older stellar population. A fainter, more diffuse halo surrounds the central region. The galaxy has a relatively high degree of rotational symmetry. There is minimal evidence of spiral arms or significant dust lanes. A small object is visible above the main galaxy body, but is not significantly distorted, likely a companion galaxy, although could be a foreground or background object. No significant signs of recent or ongoing major merger activity are apparent, however, some minor disturbances may be present. Overall, the galaxy presents a mature, relatively quiescent structure.
