The galaxy presents as a moderately inclined, elongated system, likely a spiral or lenticular galaxy viewed at an angle. The light distribution is centrally concentrated with a smooth appearance, suggesting a prominent bulge or a relatively even distribution of stars throughout the disk. The color is primarily yellowish-orange, possibly indicating an older stellar population and/or a significant amount of dust obscuration. There is a subtle hint of blue color extending along the edges of the major axis, potentially indicating ongoing star formation within the disk. No distinct spiral arm structures or prominent star-forming regions are visible within the limitations of image quality. The overall morphology appears relatively undisturbed, with no obvious signs of tidal interactions or recent mergers.
