The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a predominantly elliptical shape, leaning towards rounder, with minimal elongation. There is no obvious disk structure or spiral arms. The light distribution suggests a bulge-dominated system. 

The galaxy presents a warm, yellowish hue suggesting an older stellar population, with less ongoing star formation. There is no distinct dust lane visible. Minimal tidal disturbances or signs of recent merger activity are observed, as the structure appears largely undisturbed. There is a lack of blue star forming regions.
