The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.27. It has a smooth, symmetrical morphology, with a concentrated central bulge and a gradual decrease in luminosity outwards. There is no visible spiral structure or prominent dust lanes. The galaxy displays a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. No signs of active galactic nuclei or ongoing major star formation are readily apparent. There are no indications of any tidal disturbances, such as shells or tails, suggesting that the galaxy is not currently undergoing a major merger. There may be a faint, diffuse halo extending beyond the main body of the galaxy, but it is difficult to discern due to the image quality.
