The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.26. It has a relatively smooth, featureless morphology with no apparent spiral arms or significant dust lanes. The color profile suggests a dominant population of older stars, indicated by the redder hue, particularly concentrated towards the galactic center. The galaxy exhibits a slightly elongated shape, deviating subtly from a perfect sphere. There is a hint of ongoing star formation, but the majority of light output seems to be from an older stellar population. No signs of major mergers or significant tidal disturbances are evident.