The galaxy presents an elliptical morphology, though potentially with some disk-like characteristics. Its central region exhibits a bright, concentrated core, with a relatively smooth appearance overall. The galaxy displays a color gradient, transitioning from a more yellow/red hue in the central bulge to a somewhat bluer tint at the outer edges. There are noticeable features indicative of minor disturbances or asymmetries within the galaxy’s structure. These irregularities suggest potential interactions or ongoing minor merger events. A small, bright region or knot is observed within the galactic structure, which could represent an area of increased star formation or a compact nucleus. Overall, the galaxy appears to be in a relatively stable state, despite the potential signs of interaction.
