The galaxy presents a generally smooth morphology, with a high degree of central concentration. The shape appears largely elliptical, tending toward round, with only a subtle deviation from perfect circularity. There is no obvious disk structure or spiral arm morphology visible at this resolution. Faint tidal features are not apparent, and no large-scale disturbances or signs of an ongoing major merger are observed in the galaxy's structure. There may be a minor interaction occurring, but the evidence is tenuous based on visual inspection alone. The galaxy exhibits a yellowish-orange color, indicative of an older stellar population. The light distribution is relatively uniform throughout the main body of the galaxy, with no pronounced knots of star formation observed. 
