The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a noticeable lack of spiral arm structure. Its shape is elongated, appearing cigar-shaped. The central region displays a concentration of light, suggestive of a bulge component. There's a gradual decrease in luminosity from the core outward, blending seamlessly into the surrounding space. Color gradients are subtle, but a slightly redder hue is observed in the central region, potentially indicating an older stellar population or higher dust concentration compared to the outer regions, which possess a more muted tone. No significant tidal features or signs of major mergers are immediately apparent, although minor disturbances cannot be ruled out without further spectroscopic data. Overall, the galaxy appears relatively undisturbed and evolved.
