The galaxy presents as a centrally concentrated, largely featureless object with a smooth light distribution. Its shape appears largely round, exhibiting minimal elongation or distortion. The galaxy's core is distinctly yellow-white in color, suggesting an older stellar population dominating the central region. The outer regions of the galaxy display a subtle transition to a bluer hue, indicating the presence of younger, hotter stars in these areas, although their contribution appears to be less significant. There is no apparent spiral structure, bar, or signs of recent or ongoing major mergers. Minor disturbances are not obviously visible, though subtle irregularities may be present at a level below the image resolution. Overall, the galaxy appears to be a relatively quiescent system dominated by an older stellar population, with some evidence of ongoing, but relatively low-level, star formation in its outer regions.
