The galaxy presents as a relatively bright, elongated structure. The dominant color appears to be a yellowish-orange, with some areas appearing reddish, suggestive of an older stellar population. The galaxy seems to be an elliptical galaxy, or a disk galaxy with a large bulge, with a smooth, generally featureless appearance, showing little to no evidence of spiral arm structures. The absence of distinct features indicates a lack of significant recent merger activity or major disturbances. There is a suggestion of a central bulge, although the resolution limits a detailed analysis of its structure. The galaxy has a mass likely greater than our sun, which indicates it is an older galaxy.
