The galaxy appears to be an elliptical, cigar-shaped morphology with an estimated effective radius of roughly 7 kpc. It exhibits a relatively smooth light distribution. The main body of the galaxy is characterized by a yellow-orange hue, suggesting an older stellar population and lower star formation rate. Faint blue light is visible at the edges of the galaxy, indicating the presence of some younger, hotter stars or potentially regions of ongoing star formation, although these are not prominent. The image indicates there are no signs of major disturbances or mergers affecting the overall structure of the galaxy.
