This galaxy exhibits a relatively smooth morphology overall. The central region presents a more concentrated and rounded appearance, with a yellowish hue indicative of older stellar populations. Extending outward from this core is an elongated structure, giving the galaxy a cigar-like or spindle shape. This extended component shows a slightly bluer color, which may signify the presence of younger stars or ongoing star formation activity. There are faint signs of tidal distortion or interaction, suggesting a possible minor disturbance or past merger event. The galaxy's shape is reminiscent of a lenticular or early-type spiral viewed edge-on, but with a clear deviation from a perfect disk.
