The galaxy presents as a relatively smooth, elliptical-like structure with a slightly elongated shape, possibly tending toward a cigar-like appearance. The central region exhibits a concentrated luminosity, suggesting a substantial stellar population and/or an active galactic nucleus. The galaxy displays a predominantly reddish-yellow hue, indicating a population of older, redder stars and potentially significant dust content obscuring younger, bluer stars. There is some evidence of possible tidal disturbances or interactions, with a hint of extended, diffuse light surrounding the main body. The morphology suggests a possible ongoing or recent merger event, potentially contributing to the observed shape and disturbed features. The object exhibits a considerable mass, with a low rate of star formation, and its light is redshifted, implying a substantial distance from the observer.
