The galaxy presents an elongated, cigar-like morphology. Its central region exhibits a high surface brightness, appearing as a concentrated, bright core. The light gradually diffuses outward from the core. There is very little evidence of spiral arm structures or any significant disk component. The galaxy appears generally smooth in texture. There is no apparent merger activity occurring, but the galaxy may possess slight tidal disturbances. Judging by its colors, there appears to be active star formation. The galaxy's estimated size is approximately 4 kpc in radius. The overall color suggests a mixture of stellar populations, with younger, bluer stars likely contributing to the galaxy's overall luminosity. The galaxy is relatively distant and appears to have a significant mass.
