The galaxy appears as a smooth, elliptical structure with a distinct central bulge. The galaxy exhibits a color gradient, appearing more yellow-orange in the center and fading to blue at its edges. The overall shape is elongated, suggesting a cigar-like morphology rather than a perfectly circular form. There is no clear evidence of spiral arms or significant dust lanes. There are no obvious signs of an ongoing merger or tidal disturbances. The galaxy appears relatively isolated, without any companion galaxies in close proximity. Based on the color and smooth morphology, the galaxy likely consists of an older stellar population, with relatively low levels of ongoing star formation.
