The galaxy presents as a relatively smooth, concentrated object, likely elliptical in morphology given its apparent lack of spiral arm structures. The light profile suggests a centrally concentrated bulge, with a gradual decrease in surface brightness outward from the core. The color appears largely uniform and reddish, indicative of a stellar population dominated by older, redder stars and reduced ongoing star formation. There is no apparent dust lane or strong evidence of recent merger activity or significant tidal distortions in the image. The galaxy appears largely undisturbed, exhibiting a well-defined and symmetric structure.
