The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth overall appearance. A distinct central concentration of light is observed, fading towards the outer regions. The color appears bluish, suggesting the presence of younger stellar populations. There is a hint of disturbance in its morphology, possibly indicating an ongoing or recent interaction. The main body of the galaxy is not perfectly smooth, possibly due to internal dynamical processes. The extent of the galaxy is relatively compact. The observed features suggest this galaxy may be in a transitional phase, possibly evolving due to interactions or internal dynamics, with ongoing star formation activity.
