The galaxy presents as a moderately inclined disk. The central bulge exhibits a yellow-orange hue, suggestive of an older stellar population. Proceeding outward from the bulge, a faint, greenish disk is visible, with a slight flattening evident. The disk exhibits some irregularities, perhaps indicative of minor disturbances, such as interactions with smaller galaxies. There is no readily apparent spiral structure. Overall, the galaxy's morphology appears somewhat intermediate between elliptical and spiral, possibly a lenticular galaxy experiencing some degree of interaction.
