The galaxy presents as a generally smooth, elliptical structure. Its overall shape is elongated, exhibiting a cigar-like morphology. The central region shows a concentration of light, appearing brighter and more intensely colored than the outer regions. The color gradient suggests a population of older stars dominating the luminosity. There is a hint of a faint tidal tail or stream extending from one end of the galaxy, suggesting possible past or ongoing gravitational interactions. The galaxy does not appear to have significant dust lanes or prominent spiral arm structures.
