This galaxy presents as an elongated, disk-shaped structure, likely seen edge-on or at a high inclination. The central region appears brighter and more concentrated, indicating a prominent bulge component. The light distribution in the bulge seems relatively smooth, suggestive of an older stellar population. A flattened disk extends outwards from the bulge, although the presence of distinct spiral arms is not clearly discernible in this image. The outer regions of the disk exhibit a gradual decrease in surface brightness, indicating a fading stellar density. There appears to be some minor distortions in the disk, possibly indicating interactions or ongoing accretion events. The galaxy displays a generally redder color, implying a population dominated by older stars and lower levels of recent star formation.
