The galaxy appears as a slightly elongated, centrally concentrated object with a smooth light distribution. The central region exhibits a yellowish-orange hue, which may indicate an older stellar population. Surrounding the core, there's a fainter, more diffuse region that extends outwards. Within this fainter region, hints of bluer components can be observed at the edges, suggesting regions of younger stars, or star formation. There may also be a slight disturbance in the galaxy's morphology, like tidal tails, which could suggest an interaction with another galaxy in the past. Despite the galaxy's overall smooth appearance, there is a subtle hint of an asymmetry, possibly indicating a minor merger or tidal interaction. The overall shape is more disk-like than elliptical, however is still fairly centralized and could also just be that of a lenticular galaxy.
