The galaxy presents a generally elliptical morphology, appearing elongated with a cigar-like shape. The light distribution seems smooth, without pronounced spiral arms or significant substructure. There is a central concentration of light suggesting a nucleus or bulge. The galaxy exhibits a color gradient, appearing yellower and redder towards the center and bluer towards the outer regions. This color gradient suggests an older stellar population in the center with ongoing star formation, possibly traced by the bluer light from young, massive stars, in the outer disk or halo. There is no obvious evidence of tidal features or recent major merger events in the image.
