The galaxy presents a generally smooth morphology. It appears elliptical in shape, with a somewhat elongated profile. The light distribution is centrally concentrated, with a bright, well-defined core. The color gradient suggests an older stellar population, with a yellow-orange hue indicating the presence of evolved stars. There is little evidence of distinct spiral arms or active star-forming regions. Subtle irregularities or faint tidal features are possibly present, hinting at past interactions or minor disturbances, but require further investigation for confirmation. The galaxy does not exhibit any signs of a major ongoing merger. The overall structure suggests a galaxy that is relatively evolved.
