The galaxy appears as a moderately luminous object with a somewhat amorphous structure. Its overall color profile suggests a mix of stellar populations, with a hint of younger, bluer stars alongside older, redder ones. The galaxy exhibits signs of possible interaction or disruption. This is evidenced by a more concentrated central region along with fainter, extended features. These extended structures could potentially be tidal tails or remnants of a past or ongoing merger event with a smaller galaxy. The central region has a smoother appearance, which could indicate an older stellar population dominating the core. There appears to be evidence of star formation occuring. Given its apparent redshift, this is a galaxy observed at a considerable distance, and higher resolution data would be necessary for a more detailed morphological classification. The estimated size of the galaxy suggests a relatively average size within the general galaxy population.
