The galaxy presents as a generally smooth, elliptical-like structure. The central bulge is bright and appears yellowish-white in color, suggesting an older stellar population. Extending outwards from the bulge, there is a fainter, more diffuse halo. Faint hints of spiral arm structure are possibly present in the disk, but they are not well-defined. There is evidence of minor disturbance in the structure. Small blueish regions are observed, possibly indicating areas of star formation, although the overall star formation rate appears low. The galaxy's shape is elongated, but it doesn't deviate significantly from a round morphology. 
