The object appears to be a relatively large, elliptical galaxy at a significant distance. Its morphology appears mostly smooth, with no apparent spiral arms or significant dust lanes visible. The shape is somewhat elongated, but not highly so. The color suggests an older stellar population, leaning towards redder wavelengths, indicative of reduced ongoing star formation. There may be a minor disturbance in its structure, possibly hinting at a past or ongoing interaction with a smaller galactic companion, however, there is no clear merger event visible. The galaxy shows a concentrated center, with a gradual decrease in light intensity towards its outer edges.
