The galaxy presents as a smooth, elliptical structure with a noticeable central bulge. Its overall shape is slightly elongated, exhibiting a cigar-like appearance. The galaxy's light is dominated by a yellowish-orange hue, suggesting an older stellar population and diminished star formation activity. There is no readily discernible spiral arm structure or dust lane obscuration. No signs of major merging activity are apparent, though subtle disturbances cannot be ruled out at this resolution. The luminosity profile appears concentrated towards the center, indicative of a spheroidal stellar distribution.
