The observed galaxy presents a predominantly disk-like morphology, viewed at a significant inclination, appearing nearly edge-on from our vantage point. The central bulge region exhibits a smooth, concentrated light profile with a yellowish hue, indicative of an older stellar population. Moving outward from the core, the disk displays a bluer color gradient, suggesting ongoing star formation within the galactic plane. Subtle irregularities are observed along the disk, possibly indicating minor disturbances or interactions. No strong evidence of a major merger event is apparent, although there could be subtle signs of tidal features or minor distortions of the galactic disk. The overall structure suggests an intermediate-sized spiral or lenticular galaxy with an appreciable disk component.
