The galaxy presents a generally smooth morphology, appearing somewhat featureless in this image. It exhibits an elliptical shape, tending towards a cigar-like elongation. The light distribution suggests a central concentration of stellar density with a gradual falloff towards the edges. The galaxy's color index indicates a redder overall stellar population with signs of bluer regions embedded within the central regions of the object. These bluer regions suggest areas of possible ongoing or recent star formation. Overall, the galaxy doesn't appear to be undergoing any major mergers, although there might be some minor internal disturbances present within the light distribution of the galaxy.
