The galaxy presents a largely featureless, smooth morphology. It appears elliptical in shape, tending towards a cigar-like appearance. The galaxy's core exhibits a bright, concentrated luminosity, indicative of a relatively old stellar population. There is little evidence of spiral arm structure or active star formation regions. Subtle color variations can be observed, with the central region displaying a yellowish hue. These color variations could suggest subtle differences in the age and composition of the stellar populations present at varying radii. There are indications of a very minor disturbance in the galaxy.
