The galaxy appears as a relatively bright, elliptical or lenticular system, displaying a smooth, featureless morphology. The central bulge is prominent, exhibiting a yellowish hue, indicative of an older stellar population and lower levels of ongoing star formation. The galaxy appears to be substantially extended, with the major axis significantly longer than the minor axis. There is some evidence of a faint disk component surrounding the bulge, but it lacks prominent spiral arms or distinct features. The overall color suggests a relatively evolved galaxy, likely with a significant mass and a low specific star formation rate. There is no obvious sign of any merger activity or major disturbances in the galaxy's morphology.
