The galaxy presents as a generally smooth, elongated structure. It exhibits a cigar-like shape, with a high degree of central concentration. The color profile suggests a dominant population of older stars, with a yellowish-red hue concentrated in the central bulge. There is some indication of bluer light emanating from the outer regions. Based on the red shift this is a moderately distant galaxy. Overall the morphology is relatively undisturbed, without obvious signs of recent major mergers or tidal interactions.
