The galaxy presents as a relatively smooth, disk-like structure viewed at an oblique angle. The central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. The disk component is less distinct, though hints of a spiral structure are present with some faint blue regions suggesting younger stars. The overall morphology indicates a possible early-type spiral or lenticular galaxy, lacking prominent or well-defined spiral arms. It has an estimated diameter of roughly 5 kpc. The galaxy displays an overall round shape with an extension from the center. There appears to be a smaller merging galaxy exhibiting strong blue color. This interaction may be the source of the slight disturbance in the primary galaxy's disk.
