The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth and round morphology. It appears primarily spheroidal in shape with a high degree of central concentration. The color gradient is subtle, transitioning from a yellow-white core to a slightly redder outer region. There is no evidence of spiral arms or a prominent disk structure within the observed portion. Based on the color and smooth structure, this galaxy likely contains an older stellar population with minimal ongoing star formation. There is no significant distortion of the galaxy’s shape indicating any recent or ongoing major mergers. Minor disturbances cannot be ruled out, though no evidence of tidal tails or streams are seen in the image.
