The galaxy presents a largely smooth, elliptical morphology. Its shape is elongated, appearing cigar-shaped. The core of the galaxy exhibits a bright, concentrated luminosity, suggestive of an older stellar population. Moving outwards from the core, there is a gradual decrease in luminosity. There is minimal evidence of spiral arm structures. The galaxy shows no obvious signs of major disturbances or merging events. The color distribution is fairly uniform, with a slightly redder hue, indicative of evolved stars and limited ongoing star formation.
