The galaxy appears as a compact, centrally concentrated object. Its morphology suggests a spheroid-dominated system. The light profile is generally smooth, lacking prominent spiral arm structures or distinct morphological features. A slight elongation is noticeable, indicating a deviation from a perfectly spherical shape.

Color gradients suggest a relatively uniform stellar population, with a general reddish-yellow hue. This may indicate an older stellar population with lower ongoing star formation activity. The galaxy appears to be a relatively massive system. There is no clear evidence of tidal disturbances or ongoing major mergers in this image.
