The galaxy presents as an elliptical morphology with a smooth, largely featureless structure. Its shape is elongated, appearing cigar-shaped rather than perfectly spherical. The central region exhibits a higher concentration of light, suggesting a prominent galactic bulge. The color distribution is primarily red-shifted, indicating an older stellar population. There are hints of bluer hues in the outer regions of the galaxy, but the overall color is dominated by the redder wavelengths, suggestive of low levels of recent star formation. No major signs of disruption such as tidal tails or multiple nuclei are visually apparent, however, there is some minor irregularity in the shape possibly suggestive of minor gravitational interaction. 
