The galaxy presents an overall elongated morphology, appearing somewhat cigar-shaped. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density or perhaps an active galactic nucleus. Moving outwards from the center, the light diffuses, transitioning into fainter, extended features. There appears to be some irregularity in the outer structure, hinting at potential tidal interactions or past merger events. The color gradient suggests the presence of both older stellar populations, contributing to the redder tones, and regions of active star formation, indicated by the bluer hues in some areas. The galaxy does not display a well-defined spiral structure, but rather an amorphous distribution of light. The galaxy is relatively small and faint.
