This galaxy presents as a relatively small, elongated disk galaxy, viewed nearly edge-on. The central bulge appears prominent and smoothly rounded, exhibiting a yellowish-orange hue, which may indicate an older stellar population with lower rates of on-going star formation. The disk itself is thin and elongated, displaying faint blueish-green tinges, more concentrated in the central region, potentially indicating regions of more recent star formation. The galaxy appears undisturbed, with no signs of major mergers or tidal disruptions, though there are suggestions of minor irregularities. Overall, the galaxy appears as a well-defined, isolated system with characteristics consistent with a relatively high stellar mass and suppressed star formation activity.
