The galaxy presents as a moderately luminous object with a relatively smooth, rounded morphology. Its color profile suggests a moderate redshift. There is little evidence of strong spiral arm structures or distinct features, such as prominent dust lanes, suggesting it could be a lenticular or elliptical galaxy. The galaxy does not appear to be undergoing major merging activity, with no significant tidal tails or morphological distortions visible in this image. The generally even color distribution suggests that it is relatively passive, with a low star formation rate.
