The galaxy presents as a moderately luminous, elongated structure, indicating a likely classification as an elliptical galaxy or a lenticular galaxy viewed at an angle. The central region exhibits a high concentration of light, appearing smooth and featureless. There is a subtle color gradient, transitioning from a slightly more yellow/orange hue in the core to a fainter, bluer tinge in the outer regions. This suggests the presence of older stellar populations concentrated in the center, with perhaps younger stars inhabiting the outer disk. The overall light distribution is relatively even, with no prominent spiral arms or dust lanes visible. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers with neighboring galaxies, though a minor disturbance cannot be ruled out based on the image alone. The shape is more cigar-like.
