The galaxy presents an elliptical morphology, appearing largely smooth in structure. A concentrated central bulge exhibits a distinct reddish hue, suggesting an older stellar population. Surrounding the bulge, a more diffuse disk or halo is observed, displaying a bluer color gradient indicative of younger stars or ongoing star formation. The overall shape approximates an ellipse, with only a slight deviation towards a cigar-like shape, possibly indicating a mild tidal interaction or internal instability. While no major disturbances or prominent features are immediately apparent, there may be a subtle asymmetry present, perhaps stemming from a past minor merger event or a weak interaction with another galaxy. A lack of defined spiral arms or significant dust lanes further suggests that the system is not a spiral galaxy and confirms the overall smoothness.
