The galaxy presents as a generally smooth and centrally concentrated object. It appears elliptical in shape, although it's closer to a sphere than a cigar shape. The core exhibits a yellowish hue, suggesting an older stellar population and diminished star formation activity within that region. Moving outwards, there is a gradual shift in color to more bluish tones. The outer regions are less defined with a faint disk. There is no obvious structure, such as strong spiral arms, and no indications of tidal tails or major disturbances suggestive of recent major merger events. The galaxy could be classified as an early-type spiral galaxy.
