The galaxy presents an elliptical morphology with a smooth, diffuse light profile. The central region exhibits a bright, concentrated core that gradually diminishes in intensity towards the outer edges. The galaxy appears to have an overall yellowish hue, suggestive of an older stellar population. Subtle variations in color distribution may indicate regions of ongoing or recent star formation activity. The galaxy's structure seems largely undisturbed, with no major asymmetries or tidal features indicative of recent mergers or interactions. However, the galaxy may have a companion or other source of gravitational interaction due to the slight distortions observed. Overall, this galaxy appears as a relatively evolved system likely to be at z~0.24.
