The galaxy presents an elongated, cigar-shaped morphology, suggesting it is likely an edge-on spiral or potentially an elliptical galaxy with some degree of elongation. A prominent central bulge is observed, appearing relatively smooth and bright, concentrated in the center. Fainter light is diffused around the central region, indicating the presence of a disk or halo extending outwards from the bulge. A slight color gradient is noticed, with the central bulge exhibiting a whiter hue and the outer regions showing hints of blue or slightly redder tones, implying variations in stellar populations and potentially ongoing star formation within the galactic structure. There is a possibility of minor disturbances in the morphology, suggesting either past interactions or internal dynamic processes. Overall, the galaxy exhibits characteristics consistent with a mature system displaying elements of both spheroid and disk components.
