The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.128, indicating a significant distance. It presents a smooth, featureless morphology with a high degree of central concentration, gradually fading towards the outer regions. The shape is somewhat elongated, approximating a prolate spheroid, but not significantly cigar-shaped. There is no indication of any ongoing major or minor mergers, nor any apparent tidal disturbances or interactions with other galaxies in its immediate vicinity. The color gradient suggests a stellar population that is dominated by older stars, with a minimal presence of younger, bluer stars. The galaxy's relatively low rate of star formation supports this, as it suggests that star formation has largely ceased or is occurring at a very low level.
