The galaxy presents as an elongated structure, suggesting an edge-on or nearly edge-on orientation relative to our line of sight. A prominent central bulge is visible, exhibiting a smooth, concentrated luminosity profile. The bulge appears yellowish-white, indicating a population of older stars. A faint, extended disk is observed, appearing more blueish in color, hinting towards the presence of younger stellar populations and ongoing star formation. The disk is relatively thin and appears largely undisturbed, without any noticeable spiral arm structure or significant dust lanes. No signs of tidal disturbances, major mergers, or active galactic nuclei are apparent from this image.
