The galaxy presents as a somewhat elliptical structure, exhibiting a moderate degree of elongation. The core is characterized by a brighter, concentrated region. The surrounding galactic disk appears relatively smooth with a blue tint, which suggests the presence of a younger stellar population and ongoing star formation activity, this may also suggest there isn't much dust in the galaxy. There's no apparent structure of spiral arms or a bar, and it doesn't seem to be involved in any major merging events. There is a faint plume that may indicate a minor disturbance or tidal interaction. The overall morphology of the galaxy suggests a transitional type between a pure elliptical and a spiral galaxy, potentially an S0 or early-type spiral.
