The galaxy presents as a somewhat elliptical, luminous structure with a smooth, concentrated central region, exhibiting a yellow-orange hue. The light profile appears relatively even, lacking distinct spiral arms or prominent dust lanes. There is a subtle flattening effect visible, which contributes to the overall elliptical shape. The colour suggests a population of older stars and a reduced rate of on-going star formation. There are minor indications of possible disturbances but likely has not experienced any significant mergers recently.
