The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The luminosity appears to be highest in the central region, decreasing gradually toward the outer edges of the galaxy. A slight elongation is observable in the galaxy's shape, but it is neither distinctly disk-like nor cigar-shaped. The color distribution is relatively uniform, with a dominant yellowish hue, suggesting an older stellar population. There is no clear evidence of active star formation regions or spiral arm structures. The galaxy appears undisturbed, with no visible signs of major mergers or significant tidal distortions. Minor disturbances cannot be completely ruled out based on this image alone. The observed characteristics suggest a classification towards the elliptical end of the Hubble sequence.
