The galaxy presents as a well-defined, edge-on disk galaxy. There is an obvious central bulge, approximately 10% of the total disk diameter, that appears more luminous than the disk, which appears diffuse. The disk shows some faint color differentiation, potentially indicative of differential stellar populations or dust lanes, but the overall low resolution makes such determinations tentative. There's potentially some evidence of a small merger occurring in the form of faint light in the lower left corner. The lack of distinct features within the disk suggests a relatively smooth distribution of stellar material or the obscuring effect of dust. The galaxy's redshift indicates it is relatively nearby.
