The galaxy presents as an elongated, disk-like structure, viewed at an oblique angle. Its core region exhibits a concentrated, yellowish-white luminosity, suggestive of an older stellar population. Proceeding outward from the central bulge, the galaxy displays a diffuse, greenish-blue hue. This color gradient implies ongoing star formation within the galactic disk. There's also an indication of slight asymmetry or minor disturbance to the galaxy's overall form, but its is a clearly defined single galaxy. The overall shape suggests the galaxy is likely an elongated spiral or lenticular galaxy, with an estimated size of approximately 5 kpc.
