The galaxy presents as a moderately inclined disk galaxy, exhibiting a centrally concentrated bulge. The bulge displays a yellowish-orange hue, suggesting a population of older stars. The disk is less defined, with a smoother appearance and a slightly bluer color than the bulge. There's no clear evidence of well-defined spiral arms or significant dust lanes. The overall morphology indicates a galaxy that is mostly smooth in texture, with only minor disturbances in its structure, implying that it may not be currently undergoing a major merging event. The ellipticity of the galaxy suggests it's not perfectly face-on, but rather has a notable inclination relative to our line of sight.
