The galaxy presents a somewhat elliptical morphology. It displays a bright, concentrated central bulge that appears yellowish in color, suggesting an older stellar population dominating the core. Surrounding the bulge, there's a fainter, more diffuse disk component that exhibits a slightly bluer hue, hinting at the presence of younger, hotter stars and possibly ongoing star formation, although not at a prodigious rate. There is some indication of minor structural irregularity in the disk, possibly tidal interactions with a smaller galaxy, or internal disturbances. Overall, it seems to be an intermediate-mass galaxy, at an intermediate stage of evolution, somewhere between a spiral and an elliptical galaxy.
