The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a cigar-like shape, appearing highly elongated. A central bulge region shows a concentrated luminosity, transitioning to a more diffuse halo. The overall color profile is dominated by redder hues, with a brighter yellowish core. There is little evidence of spiral arm structures or active star-forming regions, suggesting an older stellar population. Slight color variation exists within the halo, but lacks significant features. The structure is largely undisturbed, with minimal signs of merging or tidal interactions.
