The galaxy presents as an elongated, disk-like structure, viewed at a nearly edge-on orientation. A central bulge region exhibits a concentrated, yellowish-white luminosity, suggesting a population of older stars. The disk shows bluer hues extending from the central region, which may indicate ongoing star formation activity within the spiral arms. The outer regions of the disk appear relatively smooth and thinned out, with minimal signs of prominent spiral structure or dust lanes. Overall, the galaxy appears relatively undisturbed, with no major morphological distortions indicative of recent merger activity. 
