The galaxy presents as a somewhat smooth structure with a round overall morphology, though there is some indication of irregularities and possible disturbance in its outer regions. The central region exhibits a bright, concentrated core, suggesting a significant stellar density or possibly an active galactic nucleus. The galaxy exhibits a generally smooth texture with a slight blueish hue. There may be faint tidal tails, which are indicative of gravitational interaction with another galaxy, or a past merger event. The disk component, if present, is subtle or viewed close to face-on. The lack of strong spiral arm features supports a classification as an early-type spiral or lenticular galaxy undergoing some sort of dynamic interaction.
