The galaxy presents as a luminous, disk-shaped structure with a predominantly yellow-orange hue, indicative of a significant population of older stars. The disk appears to be oriented approximately edge-on relative to our line of sight, suggested by the elongated, flattened appearance. There may be some disturbances in the form of galactic merging. A bright, compact region is observed, potentially representing the galactic nucleus, exhibiting a similar color profile to the broader disk. There is some evidence of lower luminosity in the disk, implying that this galaxy is likely a late-type spiral. There is also a brighter point on one side of the galaxy, which may indicate an area of active star formation. Overall, the galaxy appears to be a massive system undergoing some disturbance within an evolved stellar population.
