This galaxy exhibits a relatively smooth, elongated morphology. The central bulge appears luminous and concentrated, displaying a yellowish-white hue, likely indicative of an older stellar population. Fainter, bluish extensions protrude from both ends of the bulge, suggesting the presence of a disk-like structure. The lack of distinct spiral arm structures suggests that the disk is either quite smooth or observed at an angle that obscures its features. There is a hint of ongoing star formation activity within the disk, evidenced by the faint blue color. It appears to be a relatively isolated galaxy, with no major signs of tidal disruption or interaction with other galaxies. Minor disturbances may be present, but are subtle.
