The galaxy presents a mostly smooth morphology, appearing as a central bulge surrounded by a fainter disk. The bulge is significantly brighter than the disk, exhibiting an elliptical shape. The overall roundness suggests a lack of significant disturbance or ongoing major merger activity. There is a very slight blue hue in the disk, indicative of some ongoing star formation, but the galaxy is dominated by the yellow light of older stars. The faint, extended disk is relatively featureless, with no distinct spiral arm structures visible at this resolution. There are no obvious signs of tidal tails or other strong gravitational interactions.
