The galaxy presents a largely smooth morphology, with a central, highly luminous bulge dominating its structure. This central region exhibits a yellowish-orange hue, indicative of an older stellar population. There is a faint, less concentrated disk surrounding the bulge, though the overall light distribution appears concentrated toward the center of the galaxy. The disk structure appears relatively undisturbed with only minor asymmetric structure, and there is no strong evidence of recent or ongoing major merger activity. Faint bluer patches exist within the disk, likely indicating regions of more recent star formation. The galaxy appears to be a significant distance away. Overall, this galaxy appears to be an early-type spiral galaxy undergoing a relatively low rate of star formation.
