The galaxy presents as a relatively smooth, elongated structure. There is a concentrated central bulge, which appears yellowish-white, suggesting an older stellar population and/or significant dust obscuration. The outer regions exhibit a slightly bluer hue, potentially indicating the presence of younger stars or lower dust content compared to the core. There are no distinct spiral arm structures visible in the image; it presents as a lenticular galaxy. The galaxy's light distribution is fairly uniform, decreasing gradually from the core outwards. The galaxy does not appear to be undergoing any major merger events, though some faint asymmetry could suggest minor tidal interactions or disturbances. The apparent size of the galaxy on the image suggests a considerable physical extent.
