The galaxy presents a generally smooth morphology, with a central bulge that appears largely spheroidal and dominates the galaxy's luminosity. The bulge exhibits a yellowish hue, suggestive of an older stellar population. The galaxy exhibits a subtle, disk-like component extending beyond the bulge, displaying a bluer color. There is some indication of possible minor disturbance or asymmetry within the disk. There is no strong evidence of a major merger or tidal features. The galaxy displays a moderately high mass and star formation rate.
