The galaxy presents as a somewhat elongated, cigar-shaped structure with a smooth, diffuse appearance. The central region exhibits a concentrated luminosity, appearing yellowish in color, suggesting an older stellar population. Progressing outwards from the center, the light gradually fades, becoming more bluish, indicating the presence of younger stars within its disk. Overall, the galaxy does not display any strong spiral arm features or bar structures. There are no obvious signs of tidal disturbances or ongoing major mergers; the structure appears largely undisturbed. 
