This galaxy exhibits a relatively smooth morphology, with a notable central concentration of light. The galaxy's core presents a bright, almost stellar-like appearance, surrounded by a fainter, more diffuse halo.  A subtle elongation is apparent, suggesting a possible disk-like structure viewed at an angle, or perhaps an ongoing tidal interaction. The bluer color in the central region implies the presence of younger stars and ongoing star formation. There may be a hint of disturbance in the galaxy's overall structure, perhaps indicating a minor merger event.
