The galaxy presents as a moderately luminous, elongated structure with a concentrated central bulge. A faint disk component is visible extending outwards from the bulge. The color gradient transitions from a yellow-white core to a bluer hue towards the periphery of the disk. There are hints of some minor disturbances in the disk, but it does not appear to be undergoing any major merger activity. The overall morphology suggests a disk galaxy, possibly of intermediate type, exhibiting both characteristics of a spiral and an elliptical galaxy.
