This galaxy appears to be a spiral galaxy viewed at a slight incline. The central bulge is prominent and has a yellowish hue, suggesting an older stellar population. Faint spiral arms extend from the bulge, exhibiting a bluer color, indicative of younger stars and ongoing star formation. There is some evidence of minor disturbance in the disk, possibly due to interactions, though no major merger events appear to be occurring currently. The galaxy is relatively compact, with a moderate luminosity.
