This galaxy presents as a generally smooth, elongated structure, characteristic of an elliptical or lenticular galaxy seen edge-on or at a high inclination. The central region exhibits a concentrated luminosity gradient, appearing brighter and with a yellowish-red hue, indicative of an older stellar population potentially dominated by evolved red giant stars. Moving outwards from the core, the color transitions to a slightly bluer hue, suggesting the presence of some younger stars, or a subtle change in dust content. The galaxy's overall shape is markedly oblong; it lacks any clear spiral arm structure or significant dust lanes, further supporting a classification as a lenticular or elliptical galaxy. There is a subtle hint of minor disturbance.
