The galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical or lenticular morphology, possibly a disk galaxy seen at a high inclination. The central region displays a yellowish-orange hue, potentially indicating an older stellar population. The color becomes more green as it gets closer to the outside of the disk, which is also much dimmer than the center. There is no indication of spiral arm structure or prominent dust lanes. There appears to be no ongoing major merging activity or significant morphological disturbances. Overall, it shows an old smooth structure with older stars and a relatively low rate of star formation, possibly a red and dead galaxy.
