The observed galaxy appears to be a relatively smooth, elliptical or lenticular system, exhibiting a concentrated central bulge. It has a generally round morphology. No distinct spiral arms or significant dust lanes are discernible in the image, suggesting a lack of active, ongoing star formation. The galaxy exhibits a yellowish-orange color, which indicates an older stellar population dominated by redder stars and relatively low recent star formation. There is no obvious sign of any major mergers.
