This galaxy presents as an elongated, disk-like structure oriented edge-on relative to our line of sight. A central bulge is visible, appearing moderately bright and slightly boxy. The disk itself shows a smoother texture, with a lack of apparent distinct spiral arm features. The galaxy's color gradient indicates a yellowish hue in the central region, likely dominated by older stellar populations, transitioning to slightly bluer tones towards the outer disk. The absence of prominent dust lanes suggests either a relatively dust-poor environment or a homogenous distribution of dust obscuring any distinct features. There's no obvious evidence of ongoing major mergers or significant tidal disturbances, but a slight asymmetry or minor perturbation in the disk's structure cannot be ruled out at this resolution. Overall, the galaxy exhibits characteristics consistent with a relatively evolved disk galaxy.
