The galaxy presents as an elongated, disk-like structure. The central region is visibly brighter and exhibits a yellowish-white hue, suggesting an older stellar population with minimal active star formation in the core. Progressing outwards, the galaxy displays a bluish tint, implying the presence of younger, hotter stars and ongoing star formation activity in the spiral arms. The outer edges are indistinct, fading into the background. Overall the galaxy is an approximate elliptical shape. There is an indication of some arm structure, with the dust lanes running along the spiral arms. The galaxy shows minimal signs of recent major mergers or significant disturbances, although subtle asymmetries could indicate minor tidal interactions.
