The galaxy presents as a relatively smooth, elliptical structure. Its central bulge exhibits a concentrated, bright, yellowish hue, suggesting an older stellar population. The galaxy's overall shape is elongated, approaching a cigar-like form, with the major axis significantly longer than the minor axis. There is a subtle gradient in color as we move outwards from the center, transitioning from a warmer yellow to a cooler, bluish halo, implying the presence of some younger stars further from the core. There are no obvious signs of spiral arms or significant dust lanes. No major mergers or tidal disturbances are readily apparent, but there might be minor disturbances that are harder to detect.
