The galaxy appears as a relatively smooth, elongated structure, suggestive of an elliptical morphology or a lenticular galaxy seen edge-on. The central bulge is prominent and exhibits a yellowish hue, possibly indicating an older stellar population and lower levels of recent star formation within this region. Moving outwards from the central bulge, the galaxy transitions to a bluer color, hinting at the presence of younger stars or ongoing star formation. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, and it maintains a well-defined and symmetrical structure. Overall, this galaxy seems to be in a relatively quiescent state.
