This galaxy appears to be a relatively smooth, elliptical type, possibly a lenticular galaxy, given its shape. It presents a concentrated central bulge that is yellowish in color, indicating an older stellar population dominating the core. There is a faint, diffuse disk component extending outwards from the bulge, exhibiting a bluer hue, suggesting the presence of some younger stars or ongoing star formation within the disk, even if at a low rate. Overall, the galaxy displays a general lack of distinct features such as spiral arms or prominent dust lanes. There is no apparent indication of any major ongoing merger activity or significant morphological disturbance. The galaxy has a notable redshift suggesting that it is at a cosmologically significant distance.
