The galaxy exhibits a disturbed morphology, likely due to an ongoing or recent interaction. A prominent, somewhat elongated central bulge is visible, displaying a yellowish-orange hue, suggesting a population of older stars. Emanating from this central region, are extended, fainter structures. One such structure appears as a stream of bluish light extending away from the main body of the galaxy, indicating the presence of younger, hotter stars and possibly ongoing star formation. This stream could be tidal debris resulting from gravitational interactions. The galaxy appears moderately bright, with an estimated size of approximately 10 kpc, given the redshift. The overall shape appears somewhat cigar-shaped, though distorted by tidal forces.
