The galaxy presents as a somewhat elongated, elliptical morphology. There is a smooth gradient in light intensity, with a bright, concentrated central bulge. The outer regions of the galaxy display a fainter, diffuse glow. The color distribution appears relatively uniform, with a subtle reddening toward the central bulge. There is no evidence of prominent spiral arms or other distinct structural features such as dust lanes. The overall appearance suggests an evolved system, with a relatively old stellar population dominating the light output. The lack of significant morphological disturbances indicates that the galaxy has likely not experienced any major recent interactions or mergers.
