The galaxy exhibits an overall elliptical morphology, appearing somewhat cigar-shaped. The light profile indicates a centrally concentrated bulge with a smooth appearance, suggesting an older stellar population. Some evidence of a disk is present, but it does not dominate the structure. The color gradient reveals a redder hue, consistent with stars that are not actively forming, although there is a hint of bluer color in parts of the disk. The absence of strong spiral arm features or significant dust lanes further supports the classification as an elliptical galaxy. There is no apparent ongoing major merging activity. 
